Populations of low-mass black hole binaries

Details Populations of low-mass black hole binaries Populations of low-mass black hole binaries

Nov 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992apj...399..621r&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 399, no. 2, p. 621-626.

Astronomy and Astrophysics

Astronomy

24

Binary Stars, Black Holes (Astronomy), Neutron Stars, Stellar Evolution, Stellar Mass, Massive Stars, Stellar Physics

Scientific paper

The evolution of a population of massive binaries with low-mass secondaries is considered by contrasting the fate of black hole-producing systems with those leaving neutron stars. It is found that the interacting black hole binaries may be even more common than the familiar neutron star LMXBs. Certain unusual expected systems are described, and a comparison with present observations is made to determine the accuracy of predictions of this scenario.

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