The changing-type SN 2014C may come from an 11-M⊙ star stripped by binary interaction and violent eruption

Sun, N.-C. orcid.org/0000-0002-4731-9698, Maund, J.R. orcid.org/0000-0003-0733-7215 and Crowther, P.A. (2020) The changing-type SN 2014C may come from an 11-M⊙ star stripped by binary interaction and violent eruption. Monthly Notices of the Royal Astronomical Society, 497 (4). pp. 5118-5135. ISSN 0035-8711

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Item Type: Article
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© 2020 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Society. This is an author-produced version of a paper subsequently published in Monthly Notices of the Royal Astronomical Society. Uploaded in accordance with the publisher's self-archiving policy.

Keywords: stars: mass-loss; supernovae: general; supernovae: individual: 2014C
Dates:
  • Published: October 2020
  • Published (online): 5 August 2020
  • Accepted: 28 July 2020
Institution: The University of Sheffield
Academic Units: The University of Sheffield > Faculty of Science (Sheffield) > Department of Physics and Astronomy (Sheffield)
Funding Information:
Funder
Grant number
Royal Society
UF150689
Depositing User: Symplectic Sheffield
Date Deposited: 01 Apr 2020 09:06
Last Modified: 26 Nov 2020 16:31
Status: Published
Publisher: Oxford University Press
Refereed: Yes
Identification Number: 10.1093/mnras/staa2277
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