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Magnetic Braking of Ap/Bp Stars: Application to Compact Black-Hole X-Ray Binaries

Abstract:
We examine the proposal that the subset of neutron-star and black-hole X-ray binaries that form with Ap or Bp star companions will experience systemic angular-momentum losses due to magnetic braking, not otherwise operative with intermediate-mass companion stars. We suggest that for donor stars possessing the anomalously high magnetic fields associated with Ap and Bp stars, a magnetically coupled, irradiation-driven stellar wind can lead to substantial systemic loss of angular-momentum. In this paper we apply this mechanism to a specific astrophysics problem involving the formation of compact black-hole binaries with low-mass donor stars. At present, it is not understood how these systems form, given that low-mass companion stars are not likely to provide sufficient gravitational potential to unbind the envelope of the massive progenitor of the black hole during a prior `common-envelope' phase. However, in the absence of magnetic braking, such systems tend to evolve to long orbital periods. We show that, with the proposed magnetic braking properties afforded by Ap and Bp companions, such a scenario can lead to the formation of compact black-hole binaries with orbital periods, donor masses, lifetimes, and production rates that are in accord with the observations. In spite of these successes, our models reveal a significant discrepancy between the calculated effective temperatures and the observed spectral types of the donor stars. Finally, we show that this temperature discrepancy would still exist for other scenarios invoking initially intermediate-mass donor stars, and this presents a substantial unresolved mystery.
Publication status:
Published

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Publisher copy:
10.1111/j.1365-2966.2005.09907.x

Authors

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Institution:
University of Oxford
Division:
MPLS
Department:
Physics
Sub department:
Astrophysics
Role:
Author


Journal:
Monthly Notices of the Royal Astronomical Society More from this journal
Volume:
366
Issue:
4
Pages:
1415-1423
Publication date:
2005-11-28
DOI:
EISSN:
1365-2966
ISSN:
0035-8711


Keywords:
Pubs id:
pubs:25227
UUID:
uuid:f3262bc0-7d6c-47e3-940c-e0cf4a67342f
Local pid:
pubs:25227
Source identifiers:
25227
Deposit date:
2012-12-19
ARK identifier:

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