An unusually massive stellar black hole in the Galaxy

Greiner, J.; Cuby, J. G.; McCaughrean, M. J.

An unusually massive stellar black hole in the Galaxy

Authors

Greiner, J.

Cuby, J. G.

McCaughrean, M. J.

Description

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)