chandra_126 June 4th, 2002
Credit: NASA/CXC/UVa/E.Blanton et al.
Chandra's image of this distant galaxy revealed a surprising number of point-like sources that have been identified as black holes and neutron stars in binary star systems. Since black holes and neutron stars are the end state of the brightest and most massive stars, this detection shows that NGC 1553 once contained many very bright, massive stars, in marked contrast to the present population of low-mass faint stars that now dominate the galaxy. The bright central X-ray source is probably due to a supermassive black hole in the nucleus of the galaxy.
Provider: Chandra X-ray Observatory
Image Source: http://chandra.harvard.edu/photo/2002/1058/
Curator: Chandra X-ray Observatory, Cambridge, MA, USA
Image Use Policy: http://chandra.harvard.edu/photo/image_use.html
Detailed color mapping information coming soon...
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