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. (Submitted: 2020) The changing-type SN 2014C may come from an 11-M⊙ star stripped by binary interaction and violent eruption. arXiv. (Submitted)

Abstract

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Authors/Creators:
Copyright, Publisher and Additional Information: © 2020 The Author(s). For reuse permissions, please contact the Author(s).
Keywords: astro-ph.SR; astro-ph.SR; astro-ph.GA
Dates:
  • Submitted: 20 March 2020
Institution: The University of Sheffield
Academic Units: The University of Sheffield > Faculty of Science (Sheffield) > Department of Physics and Astronomy (Sheffield)
Funding Information:
FunderGrant number
Royal SocietyUF150689
Depositing User: Symplectic Sheffield
Date Deposited: 01 Apr 2020 09:06
Last Modified: 01 Apr 2020 09:31
Published Version: https://arxiv.org/abs/2003.09325v1
Status: Submitted
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