chandra_267 July 30th, 2003
Credit: NASA/CXC/MIT/D.Pooley et al.
Most of the point-like X-ray sources in these Chandra images are binary star systems containing a collapsed star, such as a neutron star or a white dwarf star, that is pulling matter off a normal companion star. A globular cluster is a spherical collection of hundreds of thousands or even millions of stars buzzing around each other in a gravitationally bound stellar beehive that is about a hundred light years in diameter. While direct, head-on collisions between stars are rare even in these crowded conditions, close encounters are frequent and can lead to the formation of X-ray emitting binary star systems.
Provider: Chandra X-ray Observatory
Image Source: http://chandra.harvard.edu/photo/2003/ngc6266/
Curator: Chandra X-ray Observatory, Cambridge, MA, USA
Image Use Policy: http://chandra.harvard.edu/photo/image_use.html
Telescope | Spectral Band | Wavelength | |
---|---|---|---|
Chandra (ACIS) | X-ray (Soft X-ray) | 1.46029411764706 nm | |
Chandra (ACIS) | X-ray (Medium X-ray) | 670.9 pm | |
Chandra (ACIS) | X-ray (Hard X-ray) | 292.1 pm | |
Chandra (ACIS) | X-ray (Soft X-ray) | 1.46029411764706 nm | |
Chandra (ACIS) | X-ray (Medium X-ray) | 670.9 pm | |
Chandra (ACIS) | X-ray (Hard X-ray) | 292.1 pm | |
Detailed color mapping information coming soon...
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