chandra_324 June 5th, 2006
Credit: NASA/UMass/Z.Li & Q.D.Wang
This color-coded Chandra image (red/low energy, green/medium energy, and blue/high energy X-rays) shows the central region of the Andromeda Galaxy where a diffuse, X-ray emitting cloud of hot gas was discovered in the midst of a collection of point-like sources. The point sources are associated with binary star systems that contain a neutron star or black hole that is pulling matter away from a normal star. The diffuse X-ray cloud is due to gas that has accumulated in the central region and been heated to millions of degrees, probably by supernova explosions. The energy input from the supernovas could also be driving gas out of the central region. This process may affect both the shape and evolution of the galaxy.
Provider: Chandra X-ray Observatory
Image Source: http://chandra.harvard.edu/photo/2006/m31/
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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