chandra_421 March 25th, 2009
Credit: X-ray (NASA/CXC/Harvard/J.Neilsen); Optical & IR (Palomar DSS2)
The inset of this graphic shows Chandra's X-ray image of GRS 1915+105 in context of a crowded field seen in optical and infrared light. Chandra observed this object eleven times over some ten years, allowing scientists to track and analyze the black hole's behavior. A jet in this system is apparently choked off periodically when a wind from the accretion disk increases. Conversely, once the wind dies down the jet can re-emerge. These results may be the first clear evidence that this class of black holes has a mechanism for regulating their growth.
Provider: Chandra X-ray Observatory
Image Source: http://chandra.harvard.edu/photo/2009/g1915/
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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