chandra_160 June 4th, 2002
Credit: NASA/CXC/UVa/C.Sarazin et al.
The Chandra image of this galaxy reveals diffuse hot gas dotted with many point-like sources that have been identified as black holes and neutron stars in binary star systems. X-radiation is emitted when material is pulled from a normal star and heated to extreme temperatures as it falls toward its black hole or neutron star companion. An unusually large number of the binary star X-ray sources in NGC 4697 are in "globular star clusters." This suggests that the extraordinarily dense environment of globular clusters may be a good place for black holes or neutron stars to capture a companion star.
Provider: Chandra X-ray Observatory
Image Source: http://chandra.harvard.edu/photo/2002/1140/
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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