Black hole outflows from Centaurus A detected
Jets and lobes emanating a from central black hole have been imaged at sub-millimeter wavelengths for the first time.
Provided by ESO, Garching, Germany
January 28, 2009
The jets and lobes emanating from Centaurus A's (NGC 5128) central black hole have been imaged at sub-millimeter wavelengths for the first time. The new data, from the Atacama Pathfinder Experiment (APEX) telescope in Chile, which is operated by the European Southern Observatory (ESO), have been combined with visible and X-ray wavelengths to produce this striking new image.
Centaurus A is Earth's nearest giant galaxy, at a distance of about 13 million light-years in the southern constellation of Centaurus. It is an elliptical galaxy, currently merging with a companion spiral galaxy, resulting in areas of intense star formation and making it one of the most spectacular objects in the sky. Centaurus A hosts an active and luminous central region, that radiates strongly at radio and X-ray wavelengths. A supermassive black hole powers all this activity.
In the image, we see the dust ring encircling the giant galaxy and the fast-moving radio jets ejected from the galaxy's center, signatures of the supermassive black hole at the heart of Centaurus A. In sub-millimeter light, we see not only the heat glow from the central dust disc, but also the emission from the central radio source and - for the first time in the sub millimeter - the inner radio lobes north and south of the disc. Measurements of this emission, which occurs when fast-moving electrons spiral around the lines of a magnetic field, reveal the material in the jet is traveling at approximately half the speed of light. In the X-ray emission, we see the jets emerging from the center of Centaurus A and, to the lower right of the galaxy, the glow where the expanding lobe collides with the surrounding gas, creating a shockwave.