Do flares in Sagittarius A* reflect the last stage of tidal capture?
Abstract
In recent years the case for the presence of 3-4 106 Msun black hole in our Galactic Center has gained strength from results of stellar dynamics observations and from the detection of several rapid X-ray and IR flares observed in the Sagittarius A* from 2000 to 2004. Here we explore the idea that such flares are produced when the central black hole tidally captures and disrupts a small body - e.g. a comet or an asteroid.
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