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The Formation and Evolution of Black-Hole Binaries

Published online by Cambridge University Press:  25 May 2016

Roger W. Romani
Roger W. Romani*
Affiliation:
Department of Physics, Stanford University, Stanford, CA 94305-4060, U.S.A.

Extract

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The presence of accreting black holes (BH) among the X-ray binaries has been recognized for many years. Traditionally, Cyg X-1 and the handful of other candidates have been thought of as cousins of the HMXB neutron star systems. Recent studies of the soft X-ray transients such as A 0620-00 have, however, shown that the dynamical evidence makes these low-mass systems very strong black-hole candidates. Further, analysis of the eventual end-states of various high-mass X-ray binaries suggest that some could end as observable BH-pulsar binaries, although the first such system is yet to be discovered.

Type
1 Binary Evolution
Information
Symposium - International Astronomical Union , Volume 165: Compact Stars in Binaries , 1996 , pp. 93 - 103
Copyright
Copyright © Kluwer 1996 

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