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O Mestre é um romance de Colm Tóibín, classificado pelo The New York Times como um dos 10 mais notáveis livros de 2004. Trata-se de um romance biográfico que utiliza alguns episódios da vida de Henry James, para fazer um sublime e delicado retrato íntimo do famoso escritor norte-americano.

Prémios
  International IMPAC Dublin Literary Award, 2006
 nomeado para o Booker Prize, 2004
 Los Angeles Times Novel of the Year, 2004
 Stonewall Book Award, 2004

O Mestre
!Mais Teoria da História na Wiki (Wikiconcurso de edição)

redpajama_set_name: RedPajamaWikipedia


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Microgaming's Virtual Reality Roulette
Microgaming is a casino game developer based on the Isle of Man. They're one of the bigger players in the industry and have developed some interesting technology over the years. In terms of roulette, Microgaming has around 10 variants including multi-player and progressive tables; you can play these roulette games for free at Microgaming Tribune.
Their latest technology is VR Roulette, which won Microgaming the Digital Gaming Innovation award at the Global Gaming Awards event last September. It game could revolutionize many gambling games online as it uses 3D VR technology. VR Roulette was presented to the public back in February at the latest International Gambling Expo under the motto "Welcome to the future." Visitors were given the chance to enter a futuristic Cryo lab and with the help of the Oculus Rift DK 2 headset and a Leap Motion 3D Controller get projected into a thrilling 3D world.
So if you are wondering what's like to play VR Roulette, Microgaming has released a video that presents this game alongside it other products. Turns out, once the headset is properly placed and activated, you're taken into a virtual space where you're greeted by a friendly robot. The animation also has the role of a dealer, hence you'll notice it spin the wheel, calling bets and acting perfectly normal as if it's a human dealer in a casual brick and mortar casino. Those visitors that wanted to minimize outside noise were given the opportunity to use headphones as well, thus reserving most of their senses for the unusual gaming experience. As it can be seen on the video, players are able to see the shape of their hand and then use it to place bets or interact with the surroundings.
When it comes to game-play and rules, the initially presented version of this game features a standard European layout. Nonetheless, considering the fact VR Roulette isn't available to players just yet, the option to see changes in the future aren't excluded. Knowing that Microgaming has many variants of the table game, fans can hope to see them all available in the operator's outer space universe.
Nonetheless, the main question that arises after the showcase of this technology is how it will be received by the online gambling community. Perhaps once headsets necessary for playing become affordable to the, games like VR Roulette will quickly become part of the online gambling culture. If that's the case, other game providers will likely develop competing games.
These types of roulette, as well as other games like slots, blackjack and so on, may be the next level in online gambling and gaming in general. As more and more people try to find solutions for keeping the comfort of their home and, at the same time, have an engaging gaming experience, virtual reality could become popular. It doesn't involve real wheel physics, but it may be fun nontheless. First, the launch of online gaming sites. Then, there were live dealer casinos directly streamed from studios all around the world. 3d virtually reality appears to be the next progression, and it wouldn't surprise me if soon after we'll see VR with live dealers.
Article by: Sunil
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redpajama_set_name: RedPajamaCommonCrawl


What Are The Causes of Pimples? How you can Get Rid of Pimples Painlessly?
2018-09-12 Oswald Rodrigues Comments Off on What Are The Causes of Pimples? How you can Get Rid of Pimples Painlessly?
Break outs can develop anybody from youngsters to adults. It may be discovered wherever in your physique. It principally developed on face, shoulders, neck, chest, again. Everybody's pores and skin has tiny holes, which get blocked by oil, micro organism, filth and when this occurs peoples could develop pimples. And when your pores and skin repeatedly affected by the sort of situation, then you could have an zits. It may be very irritating and everybody hates it. You'll attempt to do all the pieces excellent however nonetheless they'll come. They're numerous causes due to that it develops. It is principally develops on youngsters. There may be fable about pimples that they arrive due to sweets and French fries however there isn't any scientific proof on that. Pimples may be develops due to your hormones. It may be develops as a result of stress additionally Growing of air pollution additionally helps to develop zits in your face. Improve in Air air pollution can harm your pores and skin as there's lot of filth in air. Generally folks use unsuitable merchandise for his or her skins. For instance your pores and skin just isn't that a lot oily however nonetheless you might be utilizing 'oil free' pores and skin merchandise to your pores and skin this can have an effect on badly to your face. There are additionally some meals which aren't good however nonetheless you might be consuming a lot of the occasions. And a few the scientific causes are two a lot oil produce by your follicles, lifeless pores and skin cells accumulate in your pores, micro organism and filth construct up in your pores. So folks all the time demand for finest zits remedy if they've zits. There are numerous remedies for teenagers out there for treating zits. House cures are additionally out there to eliminate breakouts. A few of the simple and may be finished simply finished simply remedies are; cleansing your pores and skin on require time as it would take away extra oil and filth out of your face, shampooing your hairs repeatedly and preserving it out of your face, utilizing make-up's once they required not day by day or utilizing not pore-clogging make-up's, not touching your face, not squeezing your pimples. However this are the house cures and we all the time get forgets to comply with even when we comply with this on a regular basis generally zits does come. So for this now we have to get extra remedy from physician's suggestions. There are one zits detachable quick remedies out there that are very efficient and really painless. This remedy is hydrocolloid zits patch remedy. It's like versatile bandages manufactured from a water attracting materials connected to a skinny plastic movie. Like bandage you may straight use it to your zits. It's important to clear your pores and skin earlier than making use of this patch. Then after that connect the centre of this patch to the zits space press for Three seconds and depart it for 8-1 hours. The middle of this patch turns white in a single day it signifies that it is engaged on that spot. You need to have to make use of this for 3-Four days. This sort of remedy merchandise is offered in on-line market and it is extremely helpful. We've got to decide on hydrocolloid zits patch higher priced finest merchandise from on-line advertising shops.
Next Post:How Did Well being Care Prices Get So Excessive?


Leather Boot (ADE26006) by Pavers @ Pavers Shoes - Your Perfect Style.
These beautiful leather lace-up boots are a brilliant choice for the more casual look. A padded collar adds extra comfort, whilst the metal lace loop eyelets ensure stability and security.
A good all weather boot that looks good on a night out or just popping down the shops it's my second pair and if they last as long as the first there could be a 3rd.
Pavers shipped very quickly, and presentation in the box was first-class. The boots enjoy a deep, mid-brown colouring and good shine.
The feel of the leather denotes quality, and the price certainly represents very good value.
The look is one of very smart-casual, and could be teamed with either up-market jeans or formal trousers.
The only irritation is the laces supplied. They are broad and flat, and struggle to navigate the lace holes, owing to their breadth. Similarly, the laces are short in length, and it is a great struggle to tie them.
However, for less than £1 at most supermarkets, this minor issue can be solved with a new pair of (I suggest) round boot laces.
Overall, a boot with extremely high-class quality for the price, and I'm very happy with my purchase.
Bought these for my husband for Christmas, he loved them and said they were his favorite present, just had to order another pair to keep back as a birthday present for our 24yrs son as when he saw them he also loved them and wanted them, great boots for a verity of ages, smart yet casual and very well made.
As yet don't know they are my husbands Christmas present. I would think like any purchase I have made from pavers they will be fantastic value for money and excellent long lasting purchase.


Peter Gane Mutes feature a full fibre construction coupled with a birchwood base resulting in a beautifully warm and full sounding range of mutes known for their great response and intonation across all registers.
Hand made in much the same way as they always have been, these mutes make no compromise when it comes to quality of sound.
From piccolo Trumpet to BBb tuba and almost everything in between.


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CHLC-FM is a Class B FM station broadcasting on the frequency of 97.1 MHz using an omnidirectional antenna. The station has a hot adult contemporary format.

CHLC-FM operates a rebroadcaster in Forestville, namely CFRP-FM which broadcasts on 100.5 MHz using a directional antenna with an average effective radiated power of 3,374 watts and a peak effective radiated power of 6,000 watts (class A).

Both stations were previously on the AM band. CHLC was on 580 kHz until 1996, and CFRP was on 620 kHz until 2005.

References

External links
 www.chlc.com - FM 97,1 et FM 100,5

Hlc
Hlc
Hlc
Baie-Comeau
Year of establishment missing


After the first batch was sold out after 12 minutes yesterday, Blizzard has now announced the next time you can get your hands on some. As expected, many tickets from yesterday almost instantly appeared on sites such as ebay etc, for as much as $400+, so if you want to join in the fun on November 2nd and 3rd, and not spend quite that much, make sure to be in line and hope you're lucky this Friday!
Missed the first round of BlizzCon ticket sales? Fear not; you'll have another chance to pick some up and join us November 2–3 at the Anaheim Convention Center when the second batch goes on sale Saturday, May 12 at 10:00 a.m. PDT.
Also as a reminder, tickets to a special pre-BlizzCon dinner to benefit CHOC Children's will go on sale Wednesday, May 16 at 7 p.m. PDT. Separate tickets to the esports competition of BlizzCon Opening Week at Blizzard Arena Los Angeles in Burbank, CA go on sale Thursday, May 17 at 8 a.m. PDT. Check out the Opening Week ticket announcement for more details.
For those who want to join the fun online, the BlizzCon Virtual Ticket will give you a chance to experience the show from just about anywhere. Stay tuned for more information in the months ahead.
Are you sure about Friday?
It's time that EVERY event start requiring names at purchase of ticket and at entry to these events. Have a resale/refund market that you control. Otherwise you have a large amount of scum profiting off of your event being popular. Just have a full refund possible for the event up to a month before for people that actually cancel, stop enabling profiteering off events like this. It's gotten absolutely ridiculous.
Friday, Saturday, it's all the weekend man! :D Fixed it thanks.
You got my hopes up then dashed them against the rocks......Are you related to my ex-wife?
Dunno, but I am getting 50% of your annual income and you have to buy me shoes.
Having people posting shots of resales before the page had even loaded for some is pretty insane.
Can't imagine the nightmare at venues when they'd have to identify every single attendant at entry.
99% of venues you already have to show ID for proving you're over drinking age. Give an extra 15 seconds for them to read the name on a ticket to match the name on the ID. Done.
BlizzCon is returning to the Anaheim Convention Center on November 1 and 2. Tickets will go on sale May 4 at 10:00 a.m. PDT and May 8 at 7:00 p.m. PDT through AXS.
GET TICKETS MAY 4 AND 8 Whether you're exploring Azeroth with your closest friends, pushing the payload with trusted allies, or engaging in a friendly duel at the Tavern, your favorite games can feel like a home away from home. For a handful of days every year, the bonds people forge online manifest IRL at BlizzCon, as people from all walks of life converge in Anaheim to celebrate a shared love of games.
This year, we have some exciting updates designed to make the BlizzCon experience even more epic and memorable for everyone joining us—including a broader range of ticketing options and some new activities for attendees to rally around.
We're kicking things off a day earlier this year with what we're calling the BlizzCon Pregame Festivities, a "Welcome to BlizzCon" get-together in the plaza outside the convention center on Thursday, October 31, from 9 a.m. to 5 p.m. PDT. This casual gathering will give everyone a place to meet up and hang out with friends, enjoy food and drinks, and do a /readycheck before the main event begins Friday morning.
We're also making room for more indoor activities this year by expanding the show into Hall E on Friday and Saturday. If you've been to BlizzCon before, that's usually where registration and the BlizzCon Store resides—this year, the store's heading to the North Hall, registration is moving off-site (nearby), and we're recapturing the Hall E area to make room for some BlizzCon fun. We've got some playful plans in the works for that space, so stay tuned for more information.
And as always, BlizzCon 2019 will feature everything you've come to expect from the convention—the epic opening ceremony, developer panels across multiple stages, the Community Night contests, hands-on demos, world-class esports competition, and much more!
BlizzCon Pass – This is the core BlizzCon ticket you know and love, and what most BlizzCon attendees will want to go for. The BlizzCon Pass provides the same full general-admission access as in previous years, along with access to Thursday's BlizzCon Pregame Festivities. You'll also get the BlizzCon in-game goodies (to be announced), along with your choice of this year's BlizzCon Commemorative Collectible, which you can read more about below. Learn more about the BlizzCon Pass.
BlizzCon Portal Pass – New for 2019! – The BlizzCon Portal Pass is your gateway to an array of extras, including access to the Darkmoon Faire area on the eve of BlizzCon for a special "Night at the Faire." It also comes with convienct perks such as preferred parking, separate registration and security lines, an option to be among the first to enter the show on Friday and Saturday, a dedicated lounge for taking a load off during BlizzCon, and more. Learn more about the BlizzCon Portal Pass.
BlizzCon Benefit Dinner – Returning for 2019, the BlizzCon Benefit Dinner gives you a chance to meet and chat with developers, artists, and other folks from Blizzard the night before the show at a laid-back charity dinner—all for an exceptional cause. Your BlizzCon Benefit Dinner purchase also comes with entry to BlizzCon and all of the BlizzCon Portal Pass perks. As in past years, the net proceeds from the BlizzCon Benefit Dinner go to benefit CHOC Children's, whose mission is to nurture, advance, and protect the health and well-being of children. Learn more about the BlizzCon Benefit Dinner.
And of course, for those who can't make it to Anaheim in person, there will be ways to watch BlizzCon online, as well as get this year's commemorative in-game goodies. We'll share more information on our plans for experiencing BlizzCon at home in the future, so stay tuned.
GET TICKETS MAY 4 AND 8 AXS provides tickets for a wide variety of major events, and they're the ticket provider for our own esports events at the Blizzard Arena in Los Angeles. If you've bought BlizzCon tickets in the past, AXS's system works a bit differently from those in previous years. To learn more about the key changes and get yourself ready, check out our 5 Things You Need to Know About Buying BlizzCon 2019 Ticketsblog.
If you want to set up an AXS account in advance and save yourself a step during the ticket-buying process, you can head to the BlizzCon AXS account registration page. Alternatively, you'll have the option to log in using your Blizzard account during ticket sales, if you'd prefer.
Either way, note that once you've purchased tickets, they will be digitally delivered to you prior to the show via the AXS app, which you'll be prompted to download to your mobile device at your convenience following the ticket-purchase process.
BlizzCon 2019 just so happens to coincide with a very special anniversary. This year, we're celebrating 25 years of the Warcraft universe, and to mark the occasion we're giving away something uniquely Azerothian to BlizzCon attendees.
In place of the usual BlizzCon Goody Bag we've given out in the past, this year's BlizzCon-goers will receive their choice of a special, premium BlizzCon 2019 Commemorative Collectible—either an Orc Grunt statue or Human Footman statue—representing a quarter century of conflict and camaraderie, but mostly conflict.
We'll be producing quantities based on what people choose—so to accommodate production deadlines and have everyone's statue ready in time for pickup at BlizzCon, you'll need to decide which statue you want at the time you purchase your tickets. For those who might want to own both, the statues will be available for purchase separately during a limited pre-order window starting May 4, the same day as the first ticket sale.
Check out our BlizzCon 2019 Commemorative Collectible preview to get a closer look and learn more about making your selection.
This year's BlizzCon is shaping up to be an epic one. Whether you hail from Taipei, Tristram, Kansas, or King's Row, we can't wait to welcome you back home!
As mentioned above, Blizzard will be celebrating 25 years of Warcraft in November this year and all BlizzCon attendees will receive a BlizzCon 2019 Commemorative Collectible in addition to the usual Goody Bag. You need to decide which statue you want when you purchase your tickets. There's a Human Foortman (Alliance) statue and Orc Grunt (Horde) statue.
November 2019 marks the 25th anniversary of the Warcraft® universe, and instead of doing a typical BlizzCon® Goody Bag as we have in past years, we'd like to commemorate the occasion by providing BlizzCon attendees a distinctly Azerothian memento.
We're excited to announce that everyone who buys a ticket to attend this year's BlizzCon will receive their choice of a special BlizzCon 2019 Commemorative Collectible—one of two premium statues in the style of the Blizzard Legends series, celebrating a quarter century of Warcraft's timeless central conflict. Take up arms alongside the mighty Orc Grunt, or side with the bold Human Footman!
IMPORTANT! You'll need to decide which statue you want at the time you purchase your tickets on May 4 or May 8. We'll be producing quantities for pickup at BlizzCon based on what people choose, and locking in your selection now helps us ensure we'll have everyone's statue ready in time for the show!
Zug zug! Mark the 25th anniversary of Warcraft with this mighty axe-wielding Orc Grunt.
Ready for action! Honor the legends of Azeroth with the fierce and noble Human Footman.
Since statue choices are locked in at the time of ticket purchase, make sure to sync up with family and friends in advance to determine which one everyone wants. BlizzCon attendees will pick up their preselected statues with their badges at the show—and keep in mind that if you choose to transfer tickets (find out more), the selected statue will stay connected to that ticket.
In addition, anyone who wants either statue (or both!) will be able to purchase the Orc Grunt and Human Footman for a limited time on the Blizzard Gear Store starting May 4. Statues purchased during this window will be shipped directly to your home around the time of BlizzCon. Stay tuned for more details.
Here's to 25 years of Warcraft—we're looking forward to celebrating with you at BlizzCon!
If you want to participate in this year's community night contests (info mainly for cosplayers), Blizzard posted a list of categories for the costume contest.
Attention all cosplayers, moviemakers, artists, and other creators throughout the Blizzard community!
Each BlizzCon, we look forward to seeing you take the stage to show the world your creativity and talent. With today's announcement of BlizzCon® 2019, we wanted to give you a head's up that entries for our Community Night contests will be opening up in the next few weeks to give you as much time as possible to perfect your work.
If you've been to multiple BlizzCons, you know that we've been evolving Community Night to deliver the best show we can for everyone watching and all the contestants participating. While we're still finalizing details of this year's contests, we wanted to let you know that we're once again planning a cosplay contest and exhibition, talent contest, movie contest, and art contest, so it's safe to go ahead and get started on your creations.
Artisan Crafting: This category focuses on the fine details, recognizing skills that really shine close-up, such as meticulous tailoring and embroidery or intricate leatherworking details. Large-scale Fabrication: This category recognizes excellence creating costumes and props that are "larger than life," such as mechs, power armor, and so on. Please note that if you're planning to work on something like that, there will be size and mobility restrictions similar to last year. Weapons & Armor: This category recognizes the unique set of skills involved in crafting a battle-ready costume. Group Construction: This category is for teams of three or more people who each made significant contributions to the creation of a single costume. Outstanding Creation: This category recognizes costumes that are well-rounded and perfectly produced, or are outstanding in a way that does not fall in the other categories. Thanks as always for your passion and support, and for helping bring BlizzCon to life with your creativity. We'll have more to share with you soon.
Next up, is a compilation of 5 tips you need to know before buying a BlizzCon Pass.
BlizzCon 2019 tickets go on sale in two waves—one on May 4 and one on May 8—through AXS, and whether you're a convention veteran or trying to go for the first time, it pays to be prepared.
Several things are changing about this year's ticketing and badging process, and we've pulled together five pieces of essential BlizzCon 2019 ticket-sales intel.
When you arrive at the BlizzCon ticket page on AXS on the dates of the sale, you'll choose which of the three options you want to try to buy. Each of the three passes will have its own completely separate "Waiting Room" (more on that below!) and purchase process, so if you want to try to get all three, you'll need to enter each Waiting Room individually.
The Ticket Waiting Room Opens 30 Minutes Early AXS's ticketing system features a "Waiting Room" where people wait to find out if they're selected for a chance to buy tickets. This Waiting Room opens roughly 30 minutes prior to the official on-sale time—but don't worry too much about arriving far in advance.
Once the ticket sale officially begins, a number of people in the Waiting Room will be selected randomly for a chance to get tickets. So whether you get in the Waiting Room early or just before the sale starts, as long as tickets are available, your odds of getting tickets are the same.
If you're selected, you'll have 7 minutes to complete your purchase before tickets are released back into the available pool. AXS's Waiting Room also has measures in place to guard against ticket-buying bots (learn more).
You'll Need to Choose a Statue as You're Buying Tickets This BlizzCon, instead of having the typical Goody Bag as in past years, we're celebrating the 25th anniversary of Warcraft by giving each BlizzCon ticket purchaser their choice of one of two BlizzCon 2019 Commemorative Collectible statues—an Orc Grunt or a Human Footman—and you'll need to lock in your selection(s) as part of the ticket-buying process.
If you get through the Waiting Room, you'll immediately be presented with two options: "BlizzCon Pass with Grunt" and "BlizzCon Pass with Footman." You'll need select a quantity for each of them (up to a maximum total of 4), then click Next to advance to the next page.
So, for example, if you want to buy three BlizzCon Passes total, and want two Orc Grunt statues and one Human statue with those passes, you'd select BlizzCon Pass with Grunt x2 and BlizzCon Pass with Footman x1, then click Next.
After you click Next, you'll then simply reconfirm that you want 3 BlizzCon Passes total by clicking Find Tickets. That will take you to a new page where you fill out your billing information.
Remember, once your ticket purchase is complete, your choice of statue is locked in! When a ticket is scanned at badge pickup, the ticketholder will receive whichever statue was selected at the time of ticket purchase, even if you transfer the ticket to another guest. Speaking of which….
Transferring Tickets Is Permanent! When you purchase BlizzCon tickets, all of them will stay in your name—and in your AXS account—unless you decide to transfer one or more of them directly to your guests using AXS's Transfer option.
Unlike previous BlizzCons, where ticket buyers could edit the names of their guests at will until a specific deadline, AXS's Transfer option permanently hands the ticket over to your guest for them to manage. Your guest can then do with it as they wish (including transfer it to someone else), and you'll no longer have it in your account. Just make sure you're transferring to someone you trust!
The deadline for using the Transfer option is August 25 at 11:59 p.m. PDT.
You'll Need the AXS Mobile App to Get Into the Show To pick up your badge at registration this year, you'll need to download the AXS Mobile App. The app displays a QR code (one code for all of your tickets), which changes at regular intervals to help guard against dupes and fraud. Because of that, we won't be able to accept paper tickets, confirmation emails, or screenshots/photos of the QR code at BlizzCon registration.
After you buy your tickets, you should receive an email from AXS with instructions on how to download the app, or you can download it at any time for iPhone and Android.
If for some reason you find yourself at the show with a dead mobile device or some other unexpected issue preventing you from accessing the app, don't worry. Just head to the Solutions Desk at registration and they'll help you out.
And if you want even more nitty-gritty details, including things like lists of items you can bring into the show, registration hours, and more info on the badge-pickup process, make sure to explore all of the pages in the Event Info section of the BlizzCon website.
If you're planning to attend BlizzCon, it's a good idea to book your hotel in advance, because accommodation tends to get expensive around the time of the venue. Alternatively, you can check out Airbnb (Anaheim, CA).
We have a lot of excitement planned for you for BlizzCon 2019, but you'll eventually need to catch some zzz's while you're out here. Unfortunately, we can't let you sleep in the Anaheim Convention Center . . . so it's a good thing that nearby hotels have rooms set aside for BlizzCon attendees at special discounted rates.
Head to the BlizzCon 2019 hotel website to book your room now.
FIND A HOTEL If you're looking for a specific hotel you don't see listed yet, check back later—new housing options will be added as the show draws near!
For more information and updates that will help you on your journey to BlizzCon, keep an eye on our BlizzCon Travel page.
Finally, it's time to look at WoW Esports at BlizzCon 2019! Expect AWC and MDI Global Finals!
With the BlizzCon 2019 announcement, we wanted to give more details about the WoW esports on offer in Anaheim, California this fall. BlizzCon this year will have two days of WoW esports celebrations, with the Arena World Championship (AWC) Global Finals and Mythic Dungeon International (MDI) Global Finals sharing the World of Warcraft stage during both days of the event.
The AWC Global Finals will host eight teams at BlizzCon: five from North America/Europe, one from China, one from Asia-Pacific, and one from Latin America, all of whom will battle in a double-elimination bracket. In its 12th year and with more seasonal Cups than ever before, the AWC Global Finals are sure to deliver as new and veteran players alike fight for the championship.
The finale of the MDI will feature the top two teams from the Spring Season LAN and the top two point-earning teams from each division (based on yearly points) flying to California to race live and in person. These six teams will compete in a double-elimination bracket for the title of 2019 MDI Global Finals champions and their share of the prize pool. After making the transition in 2019 from an invitational series to a year-long, international program, our dungeon-runners will display peak performance on the biggest WoW esports stage in the world.
The prize pools for the AWC and MDI will include contributions from the sales of the Transmorpher Beacon and Lion's Pride/Horde's Might Fireworks toys. These contributions will be split down the middle, adding an equal amount of money to both prize pools. All your support for our gladiators and racers so far has been phenomenal, and we will provide an update on the final prize pools as we get closer to November.
For more information about BlizzCon 2019, head to the official BlizzCon website, and stay up to date with all things World of Warcraft by following us on Twitter.
BlizzCon returns to the Anaheim Convention Center this year and tickets will go on sale May 4.


Kemp Running for CA Gov?
Matt Drudge is just now reporting that Jack Kemp is considering a run for California. It'll be interesting to see how a Reaganite will fare out there these days, both electorially, and once he has the job.
Continue reading about Kemp Running for CA Gov?
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BBC's Gilligan NOT Anti-Iraq War?
Continue reading about BBC's Gilligan NOT Anti-Iraq War?
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size / dimensions: 15' x 9'9" x 64"
Dual sheeps foot companion roller. 4' diameter drums with 8" compaction spikes. Overall dimensions 15' long, 9'9" wide, 64" tall. This is a pull type unit. Ready to work. Shown by appt.


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Parallelogram Area and Perimeter Calculator
Parallelogram Area Calculator tool is used to calculate area, perimeter and length of the diagonal of a parallelogram.
Calculate Parallelogram Area and Perimeter
Enter Length of the long side, Base (b):
Enter Length of the short side, width (a):
Enter Length of the Height (h):
What is a Parallelograms ?
Like squares and rectangles, parallelograms are quadrilaterals: they have four sides and four interior angles. In a parallelogram those angles are not right angles, but the opposite sides must still be parallel to each other. The word "parallelogram" comes from the Greek word "parallelogrammon" (bounded by parallel lines). Rectangles, rhombuses, and squares are all parallelograms.
Perimeter of a Parallelogram
The perimeter of a parallelogram is the sum of its four sides. Since a parallelogram has two equal short sides (width, a ) and two equal long sides (base, b ), Perimeter=2a + 2b
Area of a Parallelogram
The area of a parallelogram is equal to its base (another name for length) times its height. Its height is not the same as its width: height is measured by a vertical line perpendicular (at right angles to) the base. Area=b * h
Characterizations of Parallelogram
A simple (non self-intersecting) quadrilateral is a parallelogram if and only if any one of the following statements is true:
Two pairs of opposite sides are equal in length
Two pairs of opposite angles are equal in measure
The diagonals bisect each other
One pair of opposite sides are parallel and equal in length
Adjacent angles are supplementary
Each diagonal divides the quadrilateral into two congruent triangles
The sum of the squares of the sides equals the sum of the squares of the diagonals. (This is the parallelogram law)
It has rotational symmetry of order 2
It has two lines of symmetry
Properties of a Parallelogram
Opposite sides of parallelogram are parallel.
Any line through the midpoint of a parallelogram bisects the area.
Parallelograms are quadrilaterals.
Square Rectangle Parallelogram Rhombus Trapezoid Circle Ellipse Cube Cuboid Sphere Hemisphere Cone Cylinder Pyramid Centroid Hypotenuse
© 2020 Calculators4U.com. All rights reserved.


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Cette page est une liste d'événements qui se sont produits durant l'année 2012 en Lorraine.

Éléments de contexte
  emplois salariés à vocation touristique sont recensés en Lorraine, principalement dans l'hôtellerie et la restauration. S'y ajoutent  emplois touristiques non salariés. Ce secteur représente 4 % de l'emploi salarié régional total. Un quart des emplois touristiques de la région sont concentrés autour de Metz-Amnéville, 19 % à Nancy et sa couronne.
 14 000 entreprises sont créées en Lorraine dont 62% d'auto-entreprises.
 Smart renforce ses positions à Hambach (Moselle) par un investissement de 200 millions d'€uros.
 3 départements lorrains sur 4 ont mis Nicolas Sarkozy en tête lors de l'élection présidentielle  du mois de mai.

Événements

 Les vingt-deux exemplaires de Z 11500 en service au troisième trimestre 2012 sont tous gérés par une seule Supervision technique de flotte (STF) : la « STF Lorraine ».
 La bière Duchesse de Lorraine brassée par Les Brasseurs de Lorraine obtient une médaille d'argent (catégorie bière ambrée de haute fermentation) au concours général agricole à Paris.
 Tournage à Metz, Pange, Jarny, Gorze, Gravelotte et Azannes-et-Soumazannes du film Le Tombeau de la garde de Patrick Basso
 Tournage à Amnéville du film La Clinique de l'amour de Artus de Penguern
 Tournage à Bitche du film Malgré-elles de Denis Malleval

Janvier
 1 janvier : création de l'actuelle université de Lorraine issue de la fusion de l'universités Paul Verlaine de Metz, des Nancy-I et II et de l'Institut national polytechnique de Lorraine , mettant de facto fin à chacun de ces quatre établissements.

Mai

 Mise en service de la centrale photovoltaïque de Toul-Rosières ou Parc solaire de la BA 136, centrale solaire photovoltaïque française d'une puissance de 115 à , mise en service en 2012 par EDF Énergies Nouvelles, à Rosières-en-Haye près de Toul / Nancy en Meurthe-et-Moselle dans le Grand Est. Avec ses 1,4 million de panneaux photovoltaïques sur , elle est à sa mise en service, la plus grande centrale solaire photovoltaïque d'Europe (centrales photovoltaïques en France, centrales photovoltaïques dans le monde).

 22 mai : importantes inondations dans l'agglomération de Nancy à la suite de précipitations record : Il tombe 82 millimètres en deux heures.
 25 mai : Claude Biwer, poursuivi pour « prise illégale d'intérêts », est initialement condamné en  à six mois de prison avec sursis et  euros d'amende par le tribunal de Verdun. Il fait appel auprès de la Cour d'appel de Nancy, qui confirme le jugement et le condamne à deux mois de prison avec sursis,  euros d'amende et cinq ans d'inéligibilité. Le jugement est confirmé par la cour de cassation en . Il est démissionné d'office de son poste de maire de Marville par le préfet, le .

Juin
 Fermeture de la Base aérienne 128 Metz-Frescaty.
 2 juin : dixième marche des fiertés LGBT (Gay Pride) à Metz
 10 et 17 Juin : sont élus députés à la suite des (législatives de 2012):
 de Meurthe de Moselle : Chaynesse Khirouni, élue dans la , Hervé Féron, réélu dans la , groupe socialiste, radical, citoyen et divers gauche, membre de la commission des Affaires culturelles et de l'Éducation, Christian Eckert élu dans la , Jacques Lamblin élu dans la , Dominique Potier , membre du Parti socialiste, élu député dans la  et Jean-Yves Le Déaut élu dans la
 de Meuse : Bertrand Pancher élu dans la , Jean-Louis Dumont : réélu dans la ,
 de Moselle : Aurélie Filippetti, élue dans la première circonscription de la Moselle, Gérard Terrier redevient député de la  circonscription de la Moselle, mais cette fois comme suppléant d'Aurélie Filippetti, titulaire du siège, nommée ministre de la Culture et de la Communication dans le second gouvernement de Jean-Marc Ayrault, elle ne peut conserver son mandat. La circonscription est en effet redécoupée, ce qui a obligé Aurélie Filippetti à abandonner la  circonscription pour la  redécoupée elle aussi, Denis Jacquat, réélu dans la deuxième circonscription de la Moselle,  Marie-Jo Zimmermann, élue dans la troisième circonscription de la Moselle,  Alain Marty : réélu dans la quatrième circonscription de la Moselle, il fait partie du groupe UMP, Céleste Lett : député de la 5e circonscription de la Moselle, Laurent Kalinowski, élu dans la 6e circonscription de la Moselle. Il élimine dès le 1er tour le député UMP sortant Pierre Lang, puis bat son adversaire FN Florian Philippot au second, Paola Zanetti : élue socialiste de la , Michel Liebgott, élu dans la huitième circonscription de la Moselle, Anne Grommerch, conserve son siège de députée dans la 9e circonscription de la Moselle après avoir obtenu 53,07 % des voix au second tour des élections législatives de juin 2012. Le , elle est élue vice-présidente du groupe UMP à l'Assemblée nationale.
 des Vosges :  Michel Heinrich, élu dans la première circonscription des Vosges,  Gérard Cherpion, élu dans la deuxième circonscription des Vosges,  François Vannson,  élu dans la troisième circonscription des Vosges et Christian Franqueville,  élu dans la quatrième circonscription des Vosges.

Juillet
 6 juillet : 6e étape du Tour de France 2012. Elle part d'Épernay et arrive à Metz.

 7 juillet : 7e étape du Tour de France 2012.  Elle part de Tomblaine et arrive à La Planche des Belles Filles, sommet d'une ascension inédite dans le Tour de France.

Août
 Août 2012 :
 création de Radio Campus Lorraine aussi connu sous le sigle « RCL » est une radio associative locale (catégorie A), diffusée depuis le  en Lorraine sur les fréquences temporaires  à Nancy et  à Metz consacrée à l'actualité de la vie étudiante en Lorraine. Radio Campus Lorraine est membre du réseau Radio Campus France.
 La Reine de la mirabelle est élue : Anaïs Jacob

Septembre

 21 septembre : l'Église Saint-François-d'Assise de Vandœuvre-lès-Nancy reçoit la protection des monuments historiques par arrêté du . C'est la fin d'un feuilleton sur sa transformation en centre commercial ou en fast-food.

 24 septembre au 31 octobre : procès de l'affaire des surirradiés de l'hôpital Jean-Monnet d'Épinal. Le médecin Jean-Marie Simon affirme mardi  devant le tribunal correctionnel de Paris que 12 personnes étaient décédées des suites des accidents. Le verdict rendu le  par la  correctionnelle de Paris condamne les deux praticiens à 4 ans de prison, dont 30 mois avec sursis, soit 18 mois ferme, 20 000 euros d'amende et interdiction d'exercer pour homicides et blessures involontaires et non assistance à personne en danger mais les relaxe du chef de soustraction de preuves, alors que le physicien est condamné à la même peine mais pour homicide involontaire ainsi que soustraction de preuves, mais relaxé de non assistance à personne en danger. Les autres prévenus (directrice de la Ddass, directeur de l'ARS, directeur de l'hôpital d'Épinal) ainsi que le Centre Hospitalier, personne morale, sont relaxés du chef de prévention de non assistance à personne en danger.

Octobre
 11, 12, 13 et 14 octobre : Festival international de géographie, à Saint-Dié-des-Vosges, sur le thème : Les facettes du paysage : nature, culture, économie.

Décembre
 19 décembre : sortie de Main dans la main, comédie dramatique française réalisée par Valérie Donzelli. Le film a été en partie tourné dans la Meuse.
 29 décembre : l'archiduc Christoph de Habsbourg-Lorraine épouse Mademoiselle Adelaïde Drapé-Frisch en la basilique Saint-Epvre de Nancy, le lendemain de leur mariage civil et d'une cérémonie d'hommage à ces ancêtres ducs de Lorraine, en la chapelle des Cordeliers.

Inscriptions ou classements aux titre des monuments historiques
 Château de Gerbéviller
 Papeterie de la Rochette
 Église Saint-François-d'Assise de Vandœuvre
 Château de Montbras
 Saline de Dieuze
 Manufacture vosgienne de grandes orgues
 Abbaye Saint-Pierre de Senones

Naissances

Décès

 25 octobre à Fameck : Stéphan Koziak, né le  à Vitry-sur-Orne, acteur français.

Voir aussi
 L'année 2012 dans le monde
 2012 en France, 2012 en Suisse,    2012 en Italie
 Bibliographie de la Chronologie de la Lorraine

Notes et références

Chronologie de la Lorraine
Lorraine


Within a couple of minutes the SMSBOOSTER application creates your own personalized SMS application for your private or business website. HTML skills are not essential! Configuring the SMSBOOSTER ist simple and integrating generated codes into your homepage even easier.
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Vancouver-based Indians Abroad for Pluralist India (IAPI) has condemned the recent attack on Swami Agnivesh by supporters of the Hindu nationalist Bhartiya Janata Party (BJP).
Agnivesh is a vocal critic of superstition and religious fundamentalism. He has been speaking out against growing intolerance and attacks on minorities under the BJP government in India. He was viciously beaten during his visit to Jharkhand by those affiliated with the BJP.
The attack was aimed at intimidating Agnivesh and muzzling a voice of reason. This follows a series of murders of rationalist scholars and activists by those who are seeking to turn India into a Hindu theocracy.
According to IAPI, the incident that left Agnivesh badly injured must be taken seriously in the light of the killings of Narendra Dahbolkar, Gobind Pansare, MM Kalburgi and Gauri Lankesh by the Hindu extremists.
The IAPI statement issued to the press also deplored the recent attack on the office of senior Congress Party leader Shashi Tharoor who came under sharp criticism from BJP supporters for denouncing attempts to turn India into an exclusionist Hindu state.
"Though we don't agree with the policies of the Congress party and will continue to question its secular credentials for its involvement in sectarian politics for opportunistic reasons, we believe that Tharoor should not be targeted for saying the right thing. Any act of violence to suppress the voice of those who believe in a diverse and pluralistic society must be condemned by everyone".


Hurst, C., & Hurrell, D. (2017). Where we were…where we are heading: One multiplicative journey. Australian Primary Mathematics Classroom, 22 (3), 26-32.
A journey into multiplicative thinking by three teachers in a primary school is reported. A description of how the teachers learned to identify gaps in student knowledge is described along with how the teachers assisted students to connect multiplicative ideas in ways that make sense.
This document is protected by copyright and is reproduced in this format with permission of the copyright owner(s); it may be copied and communicated for non-commercial educational purposes provided all acknowledgements associated with the material are retained.


It was on this day in 1337 that the woman we know as Julian of Norwich recovered from an uncertain but terrible illness and with it concluded her experience of a series of visions of Jesus.
Certainly a fascinating figure. A person about whom we know next to nothing, not even her name. About all we are sure of is that she lived for years as an anchorite, a solitary monastic, living at the church of St Julian in Norwich, from which we get a name for her. It would appear that she wrote the account of her visions at about the time they occurred. This document is known as the short text of the "Revelations of Divine Love." She spent many years reflecting on this and the fruit of that is the long text of the Revelations.
She hasn't been formally acknowledged as a saint within the Roman church, although many do celebrate the 13th of May as her feast. The Anglican church honors her on the 8th of May. As do some Lutherans.
Now my problem with Julian is the standard one for a Zen person when confronted with visionary experiences. If someone comes to me in my capacity as a spiritual director and tells of experiencing visions my response is, "Don't worry, it will pass." And almost always it does. I'm aware of the fact that many people who experience visions create idols of truth, usually with some seed of reality, but transformed through undue focus into a caricature of truth out of those visions that seems to lead to more sorrow than joy.
So, the caution. Don't worry. It will pass.
And, these experiences can have truth about them. In my own spiritual quest I experienced a number of these visionary experiences, makyo, if you will. The one that most rises in my heart is a vision of Jesus walking toward me and saying, "I have a great gift for you." Spreads his hands to reveal bleeding wounds, with which he then grasps my own hands, the pain of worlds birthing and dying running from his wounds into what are now mine.
I take it as makyo.
And, there is a very important part of my spiritual life that is informed by the hurt of the world that finds expression in that vision.
For her there appear to be three things that emerged. One, maybe the most important was that there was a great love in the universe, something that appeared to be able to overcome even hell. Second she saw that sin was ignorance. And third her imagery of the divine, both God and Jesus was feminine. It seems to me each of these things takes Christianity to a new place, a more valuable and if you will, truer place.
Hold these things lightly and who knows what might be revealed.
It seems to capture much of the spirit of divine vision that is useful.


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text:
Q: Парсинг txt-файлов. Вытаскивание части выражения из регулярки? Есть лог-файлы, каждый из которых соответствует определённой дате. И каждый содержит несколько тысяч строк. В файлах есть сообщения, у каждого сообщения есть время отправки.
Мне нужно посчитать количество сообщений за каждый час.
Я считываю текстовый файл построчно. И время отправки могу найти регуляркой:

    Regex regexMessageTime = new Regex(@"\d{2}:\d{2}:\d{2} <#\d{2}:\d{2}:\d{2}>[.]+:");

Что соответствует выражению: "00:00:00 <#00:00:00> текст:"
Количество сообщений в день я считаю просто по количеству совпадений с регуляркой.
Но как посчитать сообщения за каждый час?
Полагаю, нужно вытаскивать время сообщения в переменную DateTime, находить ближайшее сообщение к началу часа, т. е. к 00:00:00, и считать, пока не будет найден следующий час, т. е. ближайшее время к 01:00:00.
[Похожая проблема - из строки "00:00:00 <#00:00:00> текст:" нужно будет вытаскивать "текст" и в отдельную таблицу заносить.]
В правильном ли направлении мыслю?
Стоит искать способ вытащить время из регулярки? Или просто "вручную" парсить каждую строку и доставать время?
Как наиболее экономно это делать? Количество строк наверное может достигнуть и 15 тысяч, но более вероятно, что будет держаться между 5000 и 10000.
Заранее спасибо.

A: Берете из каждой строки первые два символа, atoi (или что там с C# для преобразования строки в число) на них и получаете целое число, которое соответствует часу. Regexp не нужен, для статистики достаточно массива на 24 элемента, которые увеличиваются если сообщение попало в конкретный час.

A: Лучше всего просто считать список и перевести его в нормальную структуру данных (например, назовём её LogEntry). Имея список этих самых LogEntry, можно сгруппировать по часам, например, при помощи LINQ:
entries.GroupBy(e => e.Date.Hour)

redpajama_set_name: RedPajamaStackExchange


text:
Council Turned Down Help With Grenfell Reaction To Avoid Looking Bad, MP Reveals
6 July 2017, 11:12 | Updated: 6 July 2017, 12:39
Housing officers from a number of London boroughs were stopped from helping with the response to the Grenfell fire because the council thought it would make them look bad.
Emma Dent-Coad is the new MP for Kensington and Chelsea, having won a surprising victory in the General Election last month.
And she said people that she had previously worked with from all over the capital were given leave from work to help organise the reaction to the tragedy.
But they were told they weren't needed - and she believes it was because they didn't want to look bad.
James O'Brien with Emma Dent-Coad. Picture: LBC
Speaking to James O'Brien, she said: "Maybe they thought it would make them look bad.
"Personal friends of mine who are housing officers, social workers from other parts of London were calling that morning saying they have been released from their jobs for however long they were needed, at least a week, and they were calling in to offer their help - 'just tell me where to go and what to do and I'll be there'.
"And those offers of help were refused. It was extraordinary."


text:
CONTOS DA MONTANHA MIGUEL TORGA PDF
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In the preface, the farewell to his given name is signed by Adolfo Rocha: Censorship raised obstacles and the project did not materialise. Pray to God that I will not be one of the candidates to the final condemnation. And Cintos spent the afternoon with iron and shovel in hand planting them.
Amid that tropical vigour, I grew too. Torga watched the show on May 28th. Adolfo Rocha emigrated to Brazil, sent by his parents. He returned to S. I do not adhere to the cruelty of the first, do not justify the sectarianism of the second, and curse the vampirism of the third. Still sitting on the judiciary bench today are the great and small Homers of all civilisations. Amazon Second Chance Pass it on, trade it in, give it a second life.
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Would you like to tell us about a lower price? He also printed the novella O Senhor Ventura. It seemed a transfigured people, at one time aware of the transcendence of the act that they would carry out and knowing of the circumstantial ambiguity that allowed it.
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Coimbra, February 24th I was denied, once again, a passport to leave Portugal. On June 1st, he took part in the first rally of the Socialist Party in Coimbra. Mysterious and unpredictable, it confounds the logic of any device.
Books by Miguel Torga (Author of Bichos)
I cling to the certainty that I tried to the limit of my strength, not seduced by the nod of any applause, but in passionate anxiety, almost somatic, that they were an expressive emergency, modest but authentic, from the matrix plasma of the motherland. He was honoured at Goethe Institut in Coimbra November 23rd. What could I do?
Retracted, entering an official hall, and after flying by helicopter in a Portuguese autumn sky, we were like the exiguous and somewhat transcendent image of two nations in dialogue, one old, completed, projected, the other younger, in process, more political reality than homeland space.
He went to a college in Estrada da Beira present-day Rua do Brazil and in two years only he finished the first five years of the general high school course.
Until number 10 Novemberhe published texts in all issues of the magazine: During the awards ceremony, on December 9th, the poet gave a speech offering to the Athenaeum the sum that he would receive, suggesting that it be used to publish the best works by young poets that had applied to the award: He published the poetry book Orfeu Rebelde [Rebel Orpheus].
Refuse they systematically, purely and simply? On September 12th, he took part in the celebration of the centenary of the abolition of the death penalty in Portugal, held in the University of Coimbra.
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Parasites of the people, the priest, the physician, the teacher and the judge, in the name of God, of knowledge, of the law or the Asclepius, would demand all forms of vassalage, beginning with the most concrete of all: Martinho de Anta and moved to Vila Nova, a borough of the municipality of Miranda do Corvo, in the district of Coimbra, where he worked as a general practitioner. He began elementary school in Escola de S. Not simple conviviality, but action.
Since childhood I try to, in every way and in all places. Be the first to review this item Amazon Best Sellers Rank: Martinho de Anta to practice as a clinician. Lisbon, March 19th […] I always exposed myself in storefronts shyly, as a contrived culprit, almost apologising to occasional readers for my boldness.
I barely finished reading the news in the newspaper, closed the door of my practice and walked around the hills.
Books by Miguel Torga
Share your thoughts with other customers. Amazon Inspire Digital Migueo Resources. And today, just, I believe that is reached zero. Diary XVI, despite the homages, the year was marked by a painful event: In the month of June he established himself as an otolaryngologist in Leiria, living in n.
On September 27th, he gave in the radio a speech to condemn the executions of five Basque citizens perpetrated by the Franco regime.
The jury even included ministers.
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text:
\section{Introduction}
``Giant molecular clouds (GMCs)'' are known to form
star clusters with both massive and low-mass stars while ``cold dark clouds''
(also called ``nearby dark clouds'', ``small molecular clouds'', or ``SMCs''; excluding ``infrared dark clouds'' here) can form only
low-mass stars in isolation \citep[e.g.][]{shu87,tur88,ber07}.
These two categories of molecular clouds have different physical properties.
Molecular clouds have hierarchical structure, and structures having sizes of the order 0.1 pc are often called ``molecular cloud cores'' or simply ``cores.''
The nonthermal motion or turbulence is dominant in cores in GMCs,
while the thermal motion is more dominant in cores in cold dark clouds \citep[e.g.][]{tur88,tat93,cas95}.
Because most stars in the Galaxy form in GMCs,
star formation from their cores is of great interest.
How do stars form from turbulent cores in GMCs?
Do turbulent cores dissipate turbulence partially or completely
before star formation?
Therefore, it is essential to observationally characterize cores in GMCs in
the turbulent environments where most stars are born.
It was theoretically suggested that cores are dynamical rather than quasistatic objects with relatively short lifetimes \citep[e.g.][]{bal03,bal07}.
If this is true, cores in GMCs cannot be quasistatic, and will be far different from
quiescent cores in cold dark clouds \citep[e.g.][]{mye83b,pin11}.
Some researchers have pointed out
that the dissipation of turbulence can initiate the star formation process \citep{mye83b,nak98,aso00}.
However, it is not well established observationally how turbulent molecular clouds form stars.  We wonder whether stars form in dynamical cores or quiescent cores, whether turbulence dissipates before star formation, and how it does.  To know how star formation occurs in GMCs, it is essential to investigate starless molecular cloud cores that might lead to star formation in near future in detail.

We take the Orion A cloud, which is the nearest and best studied GMC \citep[e.g.][]{gen89}. The overall structure is filamentary, and contains the ``$\int$-shaped filament'' (0.5 pc wide, 13 pc long) in the northern region \citep{bal87}.  \citet{joh99} mapped the $\int$-shaped filament at 450 and 850$\mu$m,
and found a chain of compact sources along a narrow ($<$ 0.14 pc) high-density filament.   The Orion A GMC has a hierarchical structure consisting of 1.4 pc-width filaments \citep{nag98} as well as 1 pc-sized clumps and 0.1 pc-sized cores \citep{bat83,bal87,cas90,tat93,ces94, chi97,tat98,lis98,aso00,joh06,ike07,tat08,tak13}.

To identify candidate starless cores close to star formation, we use chemical evolution tracers.
\citet{tat93} mapped the Orion A GMC in CS $J$ = 1$-$0 with the Nobeyama 45 m radio telescope, and cataloged 125 cores
(we use the prefix of TUKH).
\citet{tat10} made single-pointing observations toward more than 60 TUKH cores in CCS and other molecules with the Nobeyama 45 m radio telescope.  They detected CCS in molecular cloud cores in the Orion A GMC for the first time; this molecule is known as a tracer of young molecular gas in cold dark clouds through observations and chemical model calculations \citep{suz92}.
TUKH122 and TUKH083 are the most and second-most intense cores in CCS $J_N$ = 4$_3-3_2$, respectively, in
their observations.
From their data, TUKH083 is thought to be a young starless core, because it meets the category of the Carbon-Chain-Producing Regions (CCPRs) on the $N$(CCS)-$N$(NH$_3$)/$N$(CCS) diagram defined by \cite{hir09}.  On the other hand, TUKH122 is thought to be an older starless core, because it is not categorized in the CCPRs category.  \citet{tat14} mapped six TUKH cores in the Orion A GMC in N$_2$H$^+$ $J$ = 1$-$0 and CCS $J_N$ = 7$_6-6_5$ also with the Nobeyama 45 m telescope, and identified sub-peaks in these lines.  They confirmed that the column density ratio of N$_2$H$^+$ to CCS can be used as a chemical evolution tracer even in the GMCs if the gas temperature in the core does not exceed $\sim$ 25 K.
The N$_2$H$^+$ sub-peaks (TUKH122C and TUKH122D) inside the TUKH122 region have the largest $N$(N$_2$H$^+$)/$N$(CCS) column density ratios (2$-$3) among the starless sub-peaks observed by \citet{tat14}.
The ratios are close to the criterion between starless and star-forming core peaks, which means these sub-peaks are close to star formation. TUKH122
has the narrowest N$_2$H$^+$ line profiles in
their N$_2$H$^+$ core samples.
In this study, we mapped two starless cores TUKH083 and TUKH122 in the Orion A
GMC, by observing the ammonia (NH$_3$) and CCS emission to investigate the physical and chemical properties.
According to \citet{wil99}, TUKH083 and TUKH122 have
NH$_3$ rotational temperatures of 35 and $<$ 15 K,
respectively. These correspond to the kinetic temperature
$T_K$ = 60 K and $<$ 15 K, respectively by using the conversion given by \citet{dan88}.
\citet{wil99} obtained $T_K$ also from CO $J$ = 3$-$2 peak intensities to be
15 and 12 K for TUKH083 and TUKH122, respectively.
When we investigate the Herschel Observatory images, the dust continuum emission corresponding to TUKH122 is seen in Figure 2 of \citet{roy13}, but that corresponding to TUKH083 is not clear in Figure 10 of \citet{lom14} probably due to confusion in a crowded region.
According to Figure 2 of \citet{roy13}, the dust temperature toward TUKH122 is approximately 12$-$13 K.

In this work we adopt a distance of 418$\pm$6 pc based on
the work of \cite{kim08} as the best estimate; at this distance 1' corresponds to 0.12 pc

\section{Observations}

Observations were carried out by using the Karl G. Jansky Very Large Array (hereafter VLA)
of the National Radio Astronomy Observatory\footnote{The National Radio Astronomy Observatory is a facility of the National Science Foundation operated under cooperative agreement by Associated Universities, Inc.} of the United States of America in the D configuration.
The observation dates are five days between 2010 August 29 and 2010 September 9.
We observed NH$_3$ $(J, K)$ = (1, 1) at 23.694495 GHz \citep{ho83}
and
CCS $J_N$ = 4$_3-3_2$ at 45.379033 GHz \citep{yam90}
in both of the right-hand and left-hand circular polarizations,
simultaneously.
We employed the receiver front-ends for
1.3 cm K band and 0.7 cm Q band.
The tracking velocity was $v_{LSR-K}$ = 4.0 km s$^{-1}$.
The receiver back-end was the WIDAR correlator in the OSRO2 mode.
The channel width
was 15.625 kHz (corresponding to 0.197 km s$^{-1}$) for NH$_3$
and
31.25 kHz  (corresponding to 0.207 km s$^{-1}$) for CCS.
The number of the frequency channels was 256.
We observed 3C147 as the flux and bandpass calibrator.
The observed intensity is reported in terms of Jy beam$^{-1}$.
We used J0541-0541 as the phase calibrator.
Immediately before the flux, bandpass, and phase calibration,
we made pointing observations in X band toward the same calibrators.
Tables 1 and 2 list observation sessions and observational parameters.
The observed data were flagged, calibrated, and imaged (CLEANed) using
the CASA 4.1 software package.
The flux of the flux calibrator 3C147 is assumed
to be 1.783 Jy at K band and 1.0136 Jy at Q band,
from the model
of ``Perley-Butler 2010'' in CASA.
The CLEAN deconvolution was made using the simple Clark
Algorithm with the natural weighting and with UV taper.
For Q-band observations, we applied the Gaussian filter
of ``outertaper'' = 3$\farcs$0 in addition
in the CLEAN deconvolution.
The primary beam size was about 2$\arcmin$ for K band and 1$\arcmin$ for Q band.
We used the software package AIPS to plot images and spectra
to be presented in this paper.
Figures 1 and 2 show the primary beams of our interferometric observations at K band toward TUKH083 and TUKH122 superimposed on
the CS $J$ = 1$-$0 maps of \citet{tat93}.
All the interferometric maps are corrected for the primary beam response.

\section{Results}
Core TUKH122 was clearly detected in both the NH$_3$ and CCS emission.
Core TUKH083 was detected only in the NH$_3$ emission.
We have not detected the continuum emission either in K or Q bands.  The 3$\sigma$ upper limit to the continuum emission
is 1.56 mJy beam$^{-1}$ or 0.276 K for K band and  5.4 mJy beam$^{-1}$ or 0.189 K for Q band.

\subsection{TUKH122 map}
Figures 3 to 5 show NH$_3$ and CCS velocity-integrated intensity maps toward TUKH122.
Figure 4 shows the NH$_3$ map.
The NH$_3$ map shows the emission distribution elongated in the northwest-southeast direction.
The boundary shape is very smooth and oval.
The NH$_3$ emission roughly corresponds to the N$_2$H$^+$ emission observed by \cite{tat14} as TUKH122C and D.
The noise level increases outward, because the primary beam response is corrected.  All the features outside the primary beam size are noise rather than the emission.
The NH$_3$ core has some internal structure, and the southeastern side of the NH$_3$ core looks clumpy.  It might be affected by higher noise level near the edge of the primary beam to some extent, but it is likely that some internal structures are real.
We call the overall core TUKH122-n, and internal sub-cores TUKH122-n1 and n2.
The direction of the elongation of TUKH122-n is more or less in parallel with
the CS filament (P.A. $\sim$ 135$\arcdeg$)
having a width of $\sim$ 0.1 pc in Figure 2.
Table 3 lists the physical parameters of TUKH122-n, n1, and n2.  We fit two-dimensional Gaussians to the emission distribution, and derive the beam-deconvolved parameters.  $a$, $b$, and PA  are the major and minor diameters, and the position angle, respectively.
The axial ratio (minor diameter/major diameter) is 0.26, which is smaller than the typical value in cores in cold dark clouds, on the order 0.5 \citep{mye91}.
This core elongation is
also in parallel with the global filamentary shape \citep[e.g.][]{bal87,tat93} of the Orion A GMC.
The flux of the core TUKH122-n obtained through the spatial
two-dimensional Gaussian fitting is 392 mJy km s$^{-1}$.
Using the MPIfR 100m radio telescope,
\citet{wil99} observed TUKH122 in NH$_3$, and obtained
a main-beam radiation temperature of $T_R$ = 2.28 K
and an FWHM linewidth of 0.8 km s$^{-1}$, resulting in
an integrated intensity of 1.94 K km s$^{-1}$.
This corresponds to 1.64 Jy km s$^{-1}$
in their 43$\arcsec$ beam.
Then, 24\% of the single dish flux was resolved with the VLA.

Our interferometric CCS $J_N$ = 4$_3-3_2$ observations show three sub-cores, TUKH122-c1, c2, and c3 (Figure 5).
Table 3 lists them. These emission peaks coincide well with the single-dish CCS $J_N$ = 7$_6-6_5$ peaks in \citet{tat14}: TUKH122-c1 roughly corresponds to their TUKH122B, and TUKH-c2 and -c3 correspond to their TUKH122.
The sum of the TUKH122-c1, c2, and c3 flux is 209 mJy km s$^{-1}$.
The single-dish observations toward TUKH122 \citep{tat10} show that the CCS $J_N$ = 4$_3-3_2$ intensity and linewidth are $T_A^*$ = 0.47 K or $T_R$ = 0.78 K and an FWHM linewidth of 0.55 km s$^{-1}$, respectively, resulting in
an integrated intensity of 0.4 K km s$^{-1}$.
This corresponds to 1.0 Jy km s$^{-1}$ in their 38$\farcs$5 beam.
Our interferometric observations resolved 21\% of the emission.
The CCS emission was detected in two velocity bins (2 $\times$ 0.2 km s$^{-1}$) in the VLA observations.  It is hard to measure the linewidth, but it will be $\sim$ 0.4 km s$^{-1}$ or less.
The single-dish CCS observations \citep{tat14} also show the emission at R.A. (J2000.0) = 5$^h$39$^m$46$\fs$5, Dec. (J2000.0) = $-$7$\arcdeg$30$\arcmin$49$\arcsec$ (TUKH122E), although contours are not closed due to the limited observation area.
This peak is located outside the CCS observation field of the present study, but  just 30$\arcsec$ southeast from the NH$_3$ core boundary. Then the NH$_3$ core has the VLA CCS sub-cores on one side and the single-dish CCS on the other side, along its elongation.  It is most likely that the CCS emission surrounds the NH$_3$ core.
This is very similar to the cases of cores in cold dark clouds,
the N$_2$H$^+$-CCS configuration in L1544 and NH$_3$-CCS configuration in L1498 \citep{aik01,lai00}.
L1544 is a dense prestellar core exhibiting infall motions \citep{taf98}.
\cite{aik01} calculated numerical chemical models for a collapsing core, and found that models are consistent with the observations of L1544: the collapsing core has a chemically evolved N$_2$H$^+$ inner core surrounded by the chemically young CCS region. This likely also explains the NH$_3$ and CCS configuration in TUKH122.
TUKH122-n, L1544, and L1498 have similar linear sizes in pc.  We wonder about the current status of TUKH122-n regarding the core stability. From the similarity between TUKH122-n and L1544, it is possible that TUKH122-n may be unstable now, or may become unstable in near future by dissipating the remaining nonthermal motion or by accreting surrounding gas after turbulence dissipation.
Taking also into account high $N$(N$_2$H$^+$)/$N$(CCS) ratio implying an evolved starless core \citep{tat14}, it is most likely that TUKH122-n is a thermal starless core on the verge of star formation.

Our velocity resolution of 0.197 km s$^{-1}$ is insufficient to allow us to see whether TUKH122 is collapsing \citep{zho93,zho95,cho95,taf98} or has other systematic motion such as oscillation \citep{lad03,ket14,chi14}.
In the single-dish N$_2$H$^+$ spectra of \cite{tat14} at a resolution of  0.1 km s$^{-1}$  toward TUKH122, there is no hint of the blue-skewed spectrum of protostellar collapse.  However, it is highly desirable to obtain better velocity resolution data to investigate whether TUKH122 is collapsing or has other systematic motions.

\subsection{TUKH083 map}
Figure 6 shows the NH$_3$ map toward TUKH083.
The emission is very clumpy.
Table 3 lists 5 NH$_3$ sub-cores TUKH083-n1 to n5.
A feature at R.A. (J2000.0) = 5$^h$36$^m$50$\fs$5, Dec. (J2000.0) = $-$6$\arcdeg$31$\arcmin$47$\arcsec$ is located near the edge of the primary beam, and is as compact as the synthesized beam. Because its intensity is close to 3$\sigma$, we do not catalog it as reliable detection.
The overall complicated shape may suggest that the core is not dynamically
relaxed yet.
We did not detect the CCS emission toward TUKH083, although this source is the second most intense CCS $J_N$ = 4$_3-3_2$ core in \cite{tat10}.
The 3$\sigma$ upper limit at 0.4 km s$^{-1}$ resolution is 3.6 mJy beam$^{-1}$ km s$^{-1}$.
This means that the CCS $J_N$ = 4$_3-3_2$ emission toward TUKH083 is extended and resolved out in our interferometric observations.

\subsection{NH$_3$ spectra}
Figures 7 and 8 show the NH$_3$ spectra toward TUK122 and TUKH083,
respectively.
See \citet{mye83} for details of the hyperfine components of
NH$_3$ (1, 1) and their feature names (features 1 to 8).
NH$_3$ hyperfine feature 1 is located outside our effective spectral window.
NH$_3$ hyperfine feature 4 is the main component and the other
features are satellite components.
The intrinsic relative intensity of hyperfine components
is 0.52, 0.38, 0.56, 0.33, 0.48, and 0.28 for satellite features
2, 3, 5, 6, 7, and 8
with respect to the main component feature 4, respectively \citep{rydbeck77,ho83}.
Figure 7 shows the hyperfine component intensities toward TUKH122.
Hyperfine fitting tells us that the optical depth of the main component
is derived to be as large as 2.
This is in contrast with
the NH$_3$ (1, 1) spectrum obtained
toward the dark cloud core L1498 by \citet{mye83}, which looks optically thinner.
TUKH083 (Figure 8) shows only NH$_3$ hyperfine features 4 and 5, and their
observed intensity ratio is close
to the intrinsic relative intensity ratio.
Then, even the main component is optically thin.

\subsection{Velocity structure in NH$_3$}
Figures 9 and 10 show the intensity-weighted radial velocity maps toward TUKH122
and TUKH083, respectively. The radial velocity in TUKH122 is fairly constant over the core.
We investigate the velocity field toward TUKH122-n in NH$_3$
in detail.
To see the velocity structure along the elongation,
we rotate the image data anticlockwise by 33$\fdg$3 so that
the elongation becomes vertical.
Then, we average the data along the x axis
(perpendicular to the elongation), and
obtain the position-velocity diagram.
Figure 11 illustrates the position-velocity diagram of
NH$_3$ hyperfine features 7 and 8 toward TUKH122.
If all the hyperfine components are optically thin,
we expect to see spatial components
aligned parallel (horizontally) with each other.
These hyperfine components do not show such correspondence well.
Then, the optical depth probably affects the intensity distribution
in these position-velocity diagrams.
We derive the linewidth by using optically thinner line,
NH$_3$ hyperfine feature 8.
By fitting a two-dimensional Gaussian to the NH$_3$ hyperfine feature 8 in Figure 11,
we obtain an FWHM linewidth
of 0.280$\pm$0.002 km s$^{-1}$.
Deconvolved with an instrumental velocity resolution of 0.197 km s$^{-1}$,
the intrinsic FWHM linewidth is 0.20 km s$^{-1}$.
This value is close to the
thermal FWHM linewidth $\Delta v$(th) = (8(ln 2)$kT_k/m)^{1/2}$ for NH$_3$ at $T_k$ = 10 K of 0.16 km s$^{-1}$.
Here, $k$ is the Boltzmann constant, and $m$ is the mass of the molecule.
The FWHM linewidth for the mean mass per particle (2.33 a.m.u.) at 10 K is 0.44 km s$^{-1}$.
The turbulent FWHM linewidth $\Delta v$(turb) and total FWHM linewidth $\Delta v$(tot) \citep{mye83} are derived to be 0.16 and 0.47 km s$^{-1}$, respectively.
Because $\Delta v$(th) $>$ $\Delta v$(turb), TUKH122-n is thermally dominated.
If there is a velocity gradient across (perpendicular to) the elongation, it may contribute to $\Delta v$(turb), but we do not see any hint of such a gradient across the elongation.
We observe a slight velocity gradient
of 3.6 km s$^{-1}$ pc$^{-1}$ along the elongation from feature 8 in Figure 11.
Then, the specific angular momentum $J/M = (2/5) R v_{rot}$ (2/5 for a sphere) is
1.2 $\times$ 10$^{-3}$ km s$^{-1}$ pc.
This follows the empirical best-fit $J/M-R$ relationship obtained by
\citet{goo93} for $R$ = 0.03$-$0.3 pc, or is located slightly lower (smaller $J/M$).
We derive the ratio $\beta$ of rotational energy to the gravitational energy.  We adopt the definition of $\beta$
= (1/3) $\omega^2 R^3/GM$ \citep{goo93}, and obtain $\beta$ = 1.6 $\times$ 10$^{-2}$.
Here, $\omega$ is the angular speed, and $G$ is the gravitational constant.
This small value ($<<$ unity) is close to the typical value of 0.02 obtained in dark cloud cores \citep{goo93}, and indicates that the core is not rotationally supported.
Because the axial ratio of the core TUKH122-n is as small as 0.26 and rotation cannot account for core elongation,
it is likely that magnetic fields play a key role in
the core shaping of TUKH122.
\cite{nak98} has concluded that molecular clouds are magnetically supercritical.
\cite{cru99} has shown that the mass-to-magnetic flux ratio is about twice as critical, and static magnetic fields and turbulence (MHD waves) are equally important in cloud energetics.  He has concluded that magnetic fields are important in the physics of molecular clouds.  Our observations seem to be consistent with his conclusion.

Next, we look into the case of TUKH083.
Figure 12 shows the position-velocity diagram along right ascension
toward TUKH083 of NH$_3$ hyperfine feature 4.
The emission is integrated along declination within a box containing the
detected NH$_3$ emission.
Precisely, feature 4 consists of eight hyperfine components, and the two most intense components have a frequency difference corresponding to 0.32 km s$^{-1}$ \citep{rydbeck77}.
However, for the TUKH083 NH$_3$ core,
it is hard to separate hyperfine components in feature 4 because of overcrowding.

\subsection{Comparison between TUKH122, TUKH 123, and the dark cloud core L1544}
We compare the physical parameters of our cores in Orion and the dark cloud core L1544 in Taurus.
To the east of TUKH122, a cluster-forming core TUKH123 accompanying
L1641-south3 \citep{fuk89} containing six protostars \citep{meg12} is located (Figure 2).
Table 4 summarizes the physical parameters of TUKH122 and TUKH123 in the Orion A GMC, and that of L1544 in the dark cloud.
The CS $J$ = 1$-$0 data of TUKH122, and TUKH123 are taken from
\cite{tat93},
and the data of L1544 is taken from
\cite{ben89,taf98}.
We adopt the NH$_3$ rotation temperature for Orion cores from
\citet{wil99}, and converted it to the kinetic temperature $T_k$ using
the relation given by \citet{dan88}.
For TUKH122 and TUKH123, \citet{wil99} list upper limits of $T_k <$ 15 K, and
we adopted $T_k$ = 10 K assuming that they have temperatures similar to
those in cores in cold dark clouds.
Regarding the radius $R$, we adopt the HWHM (= FWHM/2) radius.
The major and minor radius at the half-maximum level are deconvolved values for the synthesized beam.
Then, the radius $R$ is calculated from a geometrical mean of the major and minor radius.
Regarding linewidth, we adopt the definition of the total linewidth $\Delta v$ (tot) from \citet{mye83b},
which takes into account the difference between the mass of the observed molecule and the mean mass per particle.
We use the virial mass instead of the LTE mass here, because the molecular abundance is not precisely known.
The virial mass is derived by using the total linewidth instead of the observed linewidth, and therefore is slightly different from those reported in \cite{tat93} and \cite{taf98}.
The gas density is derived from the radius and virial mass, and defined as $n$ = 1.2 $n$ (H$_2$) by taking into account the contribution of He.
We list the free-fall time estimated from density.
Table 4 shows that TUKH122-n in NH$_3$ and L1544 in N$_2$H$^+$ are very similar in the kinetic temperature (10 K), linear size (0.03 pc radius), and mass ($\sim$ 2 $M_{\odot}$).
It was often suggested that cores in GMCs and those in cold dark clouds are different in the physical properties \citep[e.g.][]{tur88}, but our observations revealed that the Orion A GMC contains at least one core very similar to the dark cloud core.

\section{Discussion}
\subsection{Turbulence in cores}
The NH$_3$ cores of TUKH083 and TUKH122 are embedded in the CS core observed by \citet{tat93}.
The thermal Jeans length and mass of the CS core are calculated
for the adopted kinetic temperature $T_k$ (table 3).
The virial mass of the TUKH122-n core 1.5 $M_{\odot}$ is close to
the Jeans mass in the parent turbulent CS core.
This is consistent with an idea that TUKH122-n has been formed as gravitational instability in the parent turbulent equilibrium core.

The intrinsic NH$_3$ linewidth in our interferometric observations is as small as 0.20 km s$^{-1}$.
The single-dish CCS $J_N$ = 7$_6-6_5$ and N$_2$H$^+$ linewidth
are 0.27$-$0.39 and 0.27$-$0.28 km s$^{-1}$, respectively \citep{tat14}, and are almost thermal.
On the other hand, the single-dish CS $J$ = 1$-$0 linewidth toward TUKH122 is as large as 0.83 km s$^{-1}$ \citep{tat93}.
According to \cite{tat98} the optical depth of this line is $<$ 0.9,
and therefore the linewidth will not be seriously affected.
Figure 13 shows the CS $J$ = 1$-$0 velocity channel map of \cite{tat93} toward TUKH122.
The CS emission is centered at the field center of the NH$_3$ and CCS observations, from $v_{LSR-K}$ = 3.6 to 4.2 km s$^{-1}$.  Then, it is observed as a non-thermal, turbulent core.
In our observations, the CCS emission is observed only within a range of 0.4 km s$^{-1}$ toward TUKH122,
which is close to the thermal FWHM linewidth.
These facts will imply turbulence dissipation in TUKH122: the turbulent TUKH122 CS core
($R$ = 0.18 pc, $\Delta v$(tot) = 0.94 km s$^{-1}$)
has formed the quiescent, thermal NH$_3$ core associated with CCS inside.
The viral mass and corresponding column density of the TUKH122 CS core is 33 $M_{\odot}$ and $N$ (H$_2$) = 2.2 $\times$ 10$^{21}$ cm$^{-2}$, respectively.
This column density is consistent with that obtained from dust continuum observations with the Herschel Observatory \citep{roy13}, $N$ (H$_2$) = 1.6$-$1.9 $\times$ 10$^{21}$ cm$^{-2}$ from their figure.
Furthermore, the NH$_3$ core looks dynamically relaxed, reminding
us of quasistatic evolution.
The NH$_3$ and CS cores are located in the CS filament (Figure 2).
We suggest that the turbulent equilibrium CS cores are formed from the turbulent filamentary molecular cloud due to the gravitational instability \citep{han93}, and the dynamically relaxed thermal NH$_3$ cores are then formed slowly with turbulence dissipation and gravitational instability.

Although the TUKH122 and L1544 NH$_3$ cores are very similar in terms of the kinetic temperature, linear size, and mass, they differ in terms of the mass of parent core: TUKH122 has a turbulent massive ($\sim$ 30 $M_{\odot}$) parent core observed, while L1544 has a thermal less-massive ($\sim$ 10 $M_{\odot}$) parent core.  Indeed, it is known that 0.1 pc-sized cores in the Orion A GMC have systematically larger linewidths and larger masses than similar-size cores in cold dark clouds \citep{tat93}.  It is possible that such a difference is related to an ability for GMC cores to form star clusters. In dark cloud cores, \cite{goo98,lai00} investigated the single-tracer single-cloud linewidth-size relation, and concluded that linewidth becomes coherent (thermal-motion dominated constant values against radius) on length scales less than $\sim$ 0.1 pc.  \cite{pin10} concluded that a transition to coherence occurs at 0.04 pc at B5 in the Perseus cold dark cloud.  GMC cores have different linewidth-size relation compared with dark cloud cores \cite{tat93,cas95}. Judging from Figure 6 of \cite{cas95}, the transition in GMC cores may occur at a smaller radius (0.01$-$0.1 pc).   This is consistent with our observations.

\subsection{Comparison between TUKH083 and TUKH122}
We found that TUKH083 and TUKH122 are very different in the distribution of the
NH$_3$ emission.
TUKH083 is clumpy, while TUKH122 has a smooth oval boundary.
In CCS, TUKH122 was detected in the interferometric observations, but TUKH083 was not detected.  This means that the CCS emission distribution is more compact in TUKH122 than in TUKH083.
There are two possibilities.
First, because TUKH083 is warmer than TUKH122,
different temperatures caused different core formation modes.
Second, TUKH083 is younger, and has not been dynamically relaxed yet.
From $N$(NH$_3$)/$N$(CCS) and $N$(N$_2$H$^+$)/$N$(CCS) \citep{tat10,tat14},
TUKH083 is most likely younger than TUKH122.
However, clearly we need more samples to establish the picture of core evolution in various environments in GMCs.

\section{Summary}
We mapped two starless molecular cloud cores, TUKH083 and TUKH122,
in the Orion A GMC in CCS and NH$_3$ with the VLA.  The TUKH122 NH$_3$ core (TUKH122-n) is elongated, and has a smooth oval boundary.  Where observed, the CCS emission surrounds the NH$_3$ core.  This is very similar to N$_2$H$^+$-CCS distribution in the Taurus cores L1544 and L1498.  TUKH122-n has an NH$_3$ linewidth of 0.20 km s$^{-1}$, which implies that the core is thermally supported.  The linewidth and shape of the NH$_3$ core seem to represent a dynamically relaxed quiescent core.  TUKH122-n (associated with CCS) is embedded in the parent turbulent CS core, which suggests TUKH122-n has formed through turbulence dissipation.
The parent core of TUKH122-n is three times more massive than that of L1544, which may suggest difference in the capability of forming the cluster.
The physical parameters of TUKH122-n resemble those of the L1544 NH$_3$ core.  The virial mass of the TUKH122-n core is 1.5 $M_\odot$,
and is on the order of the Jeans mass of the parent CS core.  TUKH083 was detected in NH$_3$ showing complicated distribution, but not in CCS.    The CCS emission toward TUKH083 appears to be resolved out.

\acknowledgments
K.T. is grateful to Tomoyuki Hanawa for comments on the
draft.
The authors would like to thank an anonymous referee for helpful comments.
Data analysis were carried out on the common use data analysis computer system at the Astronomy Data Center, ADC, of the National Astronomical Observatory of Japan.
M.C. was supported by
the Core Research Program of National Research Foundation
funded by the Ministry of Science, ICT and Future Planning
of the Korean government (grant number NRF-2011-0015816).
J.-E.L. was supported by the Basic Science Research Program through the National Research Foundation of Korea (NRF) funded by the Ministry of Education of the Korean government (grant number NRF-2012R1A1A2044689).

{\it Facility:} \facility{VLA}.

redpajama_set_name: RedPajamaArXiv


Given the amount of new housing that has been wished on Cranleigh, the proposal to close the CRC is l;udicrous. There are over 1200 new houses approved here, in case you had forgotten, and the idea of closing the CRC when 2400 people at least will need somewhere to take their rubbish is simply mindless. How will you deal with the fly tipping if this stupid idea goes ahead?
Don't close the CRC's, change the Government to one that understands how to run a decent country!
Just as many new homes are to be built….close the tip.Who would have thought that would be a good idea?
When completing your online feedback to SCC about the proposal to close Cranleigh Tip be aware that the scoring system is skewed to pre-defined responses. I found it better to request a paper copy to complete as did not trust the online site.
Unfortunately, since the Refuse Tip's hours and times of opening have been curtailed, together with the type of refuse accepted, the facility has become of limited use. In view of the Government and Local Authorities attitudes, there is no likelihood that the Tip will be retained. The subsequent fly-tipping which will result will be cleared up by Waverley using our taxes. The choice of Tories at both local and national elections has this outcome.
Why don't they charge £1 for each car I wonder. The excuse for closing anything to do with the council, is that it is underfunded, so that would cover the costs. I doubt if they would consider anything as simple as that though, and would probably welcome that land for even more new houses, to add to the misery of all the residents in the area.
It is clearly insane to consider closing the Cranleigh Recycling Centre. Where is one supposed to dump one's rubbish? Fly tipping will increase, which we will all pay for. I pay a huge amount of council tax and I do expect to be able to get rid of my rubbish for this sum. Moreover, given the massive amount of proposed building in the area, where on earth do the Council think that home owners will get rid of their rubbish? Are they really happy with people just dumping it at the side of the road? Making the already ghastly A281 even worse? I don't know who thought of this idea but they should be sacked forthwith.
Yes I completely agree – hope you have put all of that on the questionnaire and written to Surrey County Council with those comments. The more letters/emails of complaints they get the better.
I have also completed this 'kept very quiet' consultation, and posted about it on Facebook to encourage others to stand up for the recycling centre at Nanhurst Crossroads, Cranleigh.
Living on the A281, we are very well aware of the rubbish and fly tipping along this stretch of road. We have been on at Waverley Environmental Svs for 7 years about fly tipping outside our home, and once we got our local Councillor Kevin Deanus and MP Anne Milton involved, we suddenly began to get much quicker and more positive responses, including the recent installation of a live camera, so that the fly tippers can now be caught breaking the law, and therefore be prosecuted!
Closing the Nanhurst Recycling Centre is I'm afraid, typically greedy and short sighted of Surrey CC, and will massively increase fly tipping and littering in the area.
The population of Cranleigh is increasing very fast with all the building. And at the same some idiot proposes closing the dump.


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Espirito de Santo fact file
Facts and figures about the near 150 women golfers who are playing in this week's Espirito de Santo Trophy event
Here are some facts and figures about the nearly 150 women golfers who will battle it out for World amateur surpremacy at the Espirito de Santo Trophy at the Stellenbosch and De Zalze Golf Clubs near Cape Town this week:
NUMBER OF TEAMS – A total of 42 teams, the second-most in the history of the championship, will be participating in South Africa. Only in Puerto Rico in 2004 were there more teams (48).
FIRST TIME PARTICIPANTS – A total of nine teams, six from the continent of Africa, will be participating in the World Amateur Team Championships for the first time in 2006.
Those countries are: Bosnia and Herzegovina (men only), Botswana (men only), Bulgaria (men only), Gabon, Honduras (men only), Mauritius (men only), Morocco, Namibia (men only), and Zambia (women only).
CURTIS CUP REUNION – Two members of the USA team, Amanda Blumenherst and Jennie Lee, and five members of the Great Britain and Ireland team, Melissa Reid, Claire Coughlin, Martina Gillen, Breanna Loucks and Tricia Mangan, will be representing their countries at the World Team championships
YOUNGEST PLAYERS – Jessica Korda, of the Czech Republic, is 13 years old and the daughter of international tennis great Petr Korda. She is enrolled at the Pendleton School in Bradenton, Florida. Two of the three members of the Puerto Rico team are also 13 – Patricia Garcia of Guayanbo, and Kyle Roigis of San Juan. Monifa Sealy, of Trinidad and Tobago, is also 13. She is also a musician, having won the viola competition in the annual music festival twice. These players tie for the youngest in the championship's history with Mary Navarro of Spain (1984).
COUNTRY BY COUNTRY SNIPPITS
ARGENTINA – Maria Olivero, 32, of Buenos Aires, is playing in her ninth Espirito Santo competition. She has a two-year-old daughter and says: 'I became a house wife. I have had to learn how to cook, to wash and repair clothes and to make my little daughter's clothes. I can't recognize myself.'
BRAZIL – Cristina Baldi, 42, of Gramado, is playing in her seventh Women's World Amateur.
ENGLAND – Melissa Reid, 19, of Derby, England, played in the 2006 Curtis Cup Match against the USA and Kerry Smith, 34, of Croydon, England, won the 2004 English Championship. She works as a chef.
FINLAND – Captain Nina Johnson of Esbo, has brought her 3-year-old daughter along as a team mascot. She loves to cook and has catered a party for 120 people.
FRANCE – Melodie Bourdy is the sister of Gregory Bourdy, who represented France in the 2002 WATC, when they finished second to the USA. Gregory won the Telkcom PGA in South Africa in 2006.
ICELAND – Anna Lisa Johannsdottir, 22, of Reykjavik, is psychology major at Richmond University in London. She spent the summer as a caretaker of autistic children and plans to travel to Mozambique next summer to work with homeless children because of her interest in cross-cultural psychology.
IRELAND – Claire Coughlin, 26, of Cork, is a gym instructor and lifeguard at A leisure center. She represented Great Britain and Ireland at the 2006 Curtis Cup Match while Tricia Mangan, 32, of County Clare, is also a physical education teacher. A member of the 2006 GB&I Curtis Cup squad, she is employed at Limerick Prison.
ITALY – Laura Benazzo of Torino is serving for her eighth time as the captain of the Italian team.
JAPAN – Mika Miyazato, 16, of Tokyo is a high school student. She became the youngest champion in the history of the Japanese Women's Amateur at 14, in 2004. while Mayumi Satofuka is serving as the team captain for the seventh time.
NETHERLANDS – Marjet Van der Graff, 24, of Ryswijk, has just graduated from University this year with a degree in event management. Although she'll be concentrating on her golf, she says she might want to keep her eyes and ears open for how things operate from 'outside the ropes' as well.
SOUTH AFRICA – Sandra Winter is a self-employed physiotherapist, who will serve in a dual role as captain and physio. She played for South Africa in 2004.
Kelli Sheen, 18, who is 80% hearing impaired, is playing off a plus-three in just her 4th year in golf and Ashleigh Simon, 17, is already the veteran of one Espirito Santo Trophy event and two Women's World Cups of Golf where she distinguished herself in the company of some of the World's greatest professionals, including Annika Sorenstam.
SWEDEN – Bjorn Engstrom, who has previously been the physician for Swedish National Teams, is the captain this time.
SWITZERLAND – Sheila Gut-Lee, 32, of Zurich, is playing in her fourth World Amateur. She is a project manager in sport sponsorships for UBS while Caroline Rominger, 23, of Pontresina, is playing in her first Espirito Santo. Her brother, Martin, played for Switzerland in the men's World Amateur Team Championship in 2000, 2002 and 2004.
CHINESE TAIPEI: Ya-Ni Tseng, 17, of Tapei, has an enviable feather in her golfing cap. At age 15, she defeated Michelle Wie to win the 2004 US Women's Amateur Public Links Championship.
USA – Kimberly Kim, 15, of Arizona, won the US Women's Amateur in 2006 at age 14, making her the youngest champion in the 111-year history of the event. She also made the 36-hole cut at the 2006 US. Women's Open. She was also the runner-up at the 2006 US Women's Amateur Public Links championship.
ZAMBIA – Hilda Edwards, 50, of Lusaka, began playing golf at age 22. She is the first woman of color to represent Zambia in golf competitions and she was awarded the Meritorious Medal by the head of state for her contributions to sport in 2005. And, if your computer has trouble, you can call her because she works as an end user consultant and help desk manager in an IT department.
Melissa Nawa, 14, of Lusaka, has only been playing golf for three years. She finished second in the Zambia Ladies Open in 2006. At the All Africa Ladies Championship, she received the 'Baby Elephant' Trophy as the best junior player.
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Third or fourth year students, or graduate student status, or Instructor consent.
This offering is designed for engineering students (undergraduate and graduate) with an interest in design, invention, and the meaningful expression of creative ideas. It is intended to help students of engineering, design, applied science, and the useful arts explore and understand their critical role in the invention/creative process and ultimately yield insight on the technologist's role in wealth creation.
After an introduction to innovation from the perspective of economics and strategy, we explore the subject of invention and intellectual property. All issues relating to patents and patentability of inventions, copyrights and the protection of the expressions of ideas, trademarks and source identifiers will be reviewed and analyzed in the context of multiple engineering domains. While these domains will initially be functional (mechanical engineering, chemical engineering, industrial engineering, computer science, etc), we will explore how new combinations of traditionally functional knowledge (e.g. ME+CS, CS+CE, IE+CE…) are the fertile areas of new commercial markets and wealth creation.
Learn more about the instructor, Daniel Brown.


Silk is the invertebrates' great invention, used in a range of ways from from the protective stalks of lacewing eggs to the amazing hanging threads of New Zealand's 'glow worms'. Spiders, though, have taken silk-spinning to extremes. The common wolf spider has no web, but the female is a gentle parent, encasing her eggs in silk and carrying the precious bundle wherever she goes. The bolas spider uses a ball of sticky silk soaked in a copy of moth pheromone to lure its prey. Millions of communal spiders live and feed together in a vast, towering web - an arachnophobe's nightmare.