Journal article
Evolution of intermediate-mass X-ray binaries driven by magnetic braking of Ap/Bp stars: I. Ultracompact X-ray binaries
- Abstract:
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It is generally believed that ultracompact X-ray binaries (UCXBs) evolved from binaries consisting of a neutron star accreting from a low-mass white dwarf(WD) or helium star where mass transfer is driven by gravitational radiation. However, the standard WD evolutionary channel cannot produce the relatively long-period (40–60 minutes) UCXBs with ahigh time-averaged mass-transfer rate. In this work, we explore an alternative evolutionary route toward UCXBs, where the companions evolve from int...
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- Publication status:
- Published
- Peer review status:
- Peer reviewed
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(Version of record, pdf, 767.2KB)
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- Publisher copy:
- 10.3847/0004-637X/830/2/131
Authors
Funding
University of Henan Province
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China Scholarship Council
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Bibliographic Details
- Publisher:
- Institute of Physics Publisher's website
- Journal:
- Astrophysical Journal Journal website
- Volume:
- 830
- Issue:
- 2
- Pages:
- 131
- Publication date:
- 2016-10-01
- Acceptance date:
- 2016-08-08
- DOI:
- ISSN:
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1538-4357
Item Description
- Keywords:
- Pubs id:
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pubs:638436
- UUID:
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uuid:4a876a0a-3421-49c8-8d99-6632316158d2
- Local pid:
- pubs:638436
- Source identifiers:
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638436
- Deposit date:
- 2017-01-11
Terms of use
- Copyright holder:
- American Astronomical Society
- Copyright date:
- 2016
- Notes:
- © 2016. The American Astronomical Society. All rights reserved.
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