Formation and Evolution of Black Hole X-ray Transient Systems
Abstract
We study the formation of low-mass black hole X-ray binaries with main sequence companions that have formed through case C mass transfer (mass transfer following the helium core burning phase of the black hole progenitor). We identify these objects with the observed soft X-ray transients. Although this scenario requires a set of fine tuned conditions, we are able to produce a current Galactic population of about 2000 objects, in agreement with estimates based on observations. The narrow interval in initial separations leading to case C mass transfer, combined with the allowed narrow range of separations after the common envelope evolution, constrains the common envelope efficiency in this scenario: $\lambda \alpha_{ce} \approx 0.2-0.5$.
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All Related Versions
- Version 1, 2001-02-01, ArXiv
- Version 2, 2001-05-09, ArXiv
- Published version: New Astronomy, 6 (5), 331.
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