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Episodic mass ejections from common-envelope objects

Abstract:

After the initial fast spiral-in phase experienced by a common-envelope binary, the system mayenter a slow, self-regulated phase, possibly lasting hundreds of years, in which all the energy released by orbital decay can be efficiently transported to the surface, where it is radiated away.If the remaining envelope is to be removed during this phase, this removal must occur throughsome as-yet-undetermined mechanism. We carried out 1D hydrodynamic simulations of alow-mass red giant undergoing a ...

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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/stx1290

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Institution:
University of Oxford
Division:
MPLS Division
Department:
Physics; Astrophysics
Role:
Author
ORCID:
0000-0003-3595-4712
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Institution:
University of Oxford
Division:
MPLS Division
Department:
Physics; Astrophysics
Oxford college:
St Edmund Hall
Role:
Author
More by this author
Role:
Author
ORCID:
0000-0001-6251-5315
Canada Research Chairs More from this funder
Natural Sciences and Engineering Research Council of Canada More from this funder
Chinese Academy of Sciences More from this funder
National Natural Science Foundation of China More from this funder
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Publisher:
Oxford University Press Publisher's website
Journal:
Monthly Notices of the Royal Astronomical Society Journal website
Volume:
470
Issue:
2
Pages:
1788-1808
Publication date:
2017-05-05
Acceptance date:
2017-05-21
DOI:
EISSN:
1365-2966
ISSN:
0035-8711
Pubs id:
pubs:698372
URN:
uri:9ad678ba-12da-4031-8c7a-6dfd322277de
UUID:
uuid:9ad678ba-12da-4031-8c7a-6dfd322277de
Local pid:
pubs:698372

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