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A common-envelope wind model for Type Ia supernovae – I. Binary evolution and birth rate

Abstract:

The single-degenerate (SD) model is one of the principal models for the progenitors of type Ia supernovae (SNe Ia), but some of the predictions in the most widely studied version of the SD model, i.e. the optically thick wind (OTW) model, have not been confirmed by observations. Here, we propose a new version of the SD model in which a common envelope (CE) is assumed to form when the mass-transfer rate between a carbon-oxygen white dwarf (CO WD) and its companion exceeds a critical accretion ...

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Publication status:
Published
Peer review status:
Peer reviewed
Version:
Publisher's version

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Publisher copy:
10.1093/mnras/stx1137

Authors


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Institution:
University of Oxford
Division:
MPLS Division
Department:
Physics; Astrophysics
Oxford college:
St Edmund Hall
Role:
Author
Natural Science Foundation of China More from this funder
Chinese Academy of Sciences More from this funder
Publisher:
Oxford University Press Publisher's website
Journal:
Monthly Notices of the Royal Astronomical Society Journal website
Volume:
469
Issue:
4
Pages:
4763-4787
Publication date:
2017-05-05
Acceptance date:
2017-05-09
DOI:
EISSN:
1365-2966
ISSN:
0035-8711
Pubs id:
pubs:696535
URN:
uri:0f9fee87-703b-496d-ada1-df59d5d43b0f
UUID:
uuid:0f9fee87-703b-496d-ada1-df59d5d43b0f
Local pid:
pubs:696535

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