Journal article
Subdwarf B stars from the common envelope ejection channel
- Abstract:
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Context
Subdwarf B stars (sdB) are important to stellar evolutionary theory and asteroseismology, and are crucial to our understanding of the structure and evolution of the Galaxy. From the canonical binary scenario, the majority of sdBs are produced from low-mass stars with degenerate cores where helium is ignited in a way of flashes. Due to numerical difficulties, the models of produced sdBs are generally constructed from more massive stars with non-degenerate cores. This leave...
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- Publication status:
- Published
- Peer review status:
- Peer reviewed
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- Files:
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(Preview, Version of record, pdf, 961.1KB, Terms of use)
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- Publisher copy:
- 10.1051/0004-6361/201629622
Authors
Funding
Bibliographic Details
- Publisher:
- EDP Sciences
- Journal:
- Astronomy & Astrophysics More from this journal
- Volume:
- 54
- Pages:
- A54
- Publication date:
- 2017-02-01
- Acceptance date:
- 2017-01-05
- DOI:
- EISSN:
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1432-0746
- ISSN:
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0004-6361
Item Description
- Keywords:
- Pubs id:
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pubs:641897
- UUID:
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uuid:353edc58-6ebc-4637-b165-d2500ea3dc71
- Local pid:
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pubs:641897
- Source identifiers:
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641897
- Deposit date:
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2017-01-11
Terms of use
- Copyright holder:
- European Space Organisation
- Copyright date:
- 2017
- Notes:
- © ESO 2017
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