Investigating the origin of the spectral line profiles of the Hot Wolf-Rayet Star WR 2

Chené, A.-N., St-Louis, N. orcid.org/0000-0003-3890-3400, Moffat, A.F.J. et al. (11 more authors) (2019) Investigating the origin of the spectral line profiles of the Hot Wolf-Rayet Star WR 2. Monthly Notices of the Royal Astronomical Society. ISSN 0035-8711

Abstract

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Authors/Creators:
Copyright, Publisher and Additional Information: © 2019 The Author(s). 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: individual: WR 2; stars: Wolf-Rayet; stars: winds; outflows; stars: rotation; stars: magnetic fields
Dates:
  • Published (online): 11 February 2019
Institution: The University of Sheffield
Academic Units: The University of Sheffield > Faculty of Science (Sheffield) > Department of Physics and Astronomy (Sheffield)
Depositing User: Symplectic Sheffield
Date Deposited: 18 Feb 2019 12:05
Last Modified: 18 Feb 2019 12:05
Published Version: https://doi.org/10.1093/mnras/stz411
Status: Published online
Publisher: Oxford University Press
Refereed: Yes
Identification Number: https://doi.org/10.1093/mnras/stz411

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