An unusually massive stellar black hole in the Galaxy

Abstract

Here we report a measurement of the orbital period and mass function of GRS 1915+105 which allow us to deduce a mass of 14 +- 4 solar masses for its black hole. This large mass provides a challenge for black hole formation scenarios in binaries, since black holes with masses above 5-7 solar masses are hard to explain. Also, the mass estimate allows us to understand the unique X-ray variability of GRS 1915+105 as being due to instabilities of a radiation-pressure dominated disk radiating near the Eddington limit. Finally, several models are constrained which relate observable X-ray properties to the spin of black holes in microquasars. Once further calibrated, these relations may soon turn into a valuable tool to study relativistic effects in strong gravitational fields.

appeared in Nature 414, p. 522 (Nov. 29, 2001)

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• Formation of High Mass X-ray Black Hole Binaries
• Donor Stars in Black-Hole X-Ray Binaries
• The Formation of High-Mass Black Holes in Low Mass X-ray Binaries
• RXTE Spectroscopy of GRS 1915+105

Cited by in corpus (203)

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