Testing the fossil field hypothesis: could strongly magnetised OB stars produce all known magnetars?

Makarenko, EI, Igoshev, AP orcid.org/0000-0003-2145-1022 and Kholtygin, AF (2021) Testing the fossil field hypothesis: could strongly magnetised OB stars produce all known magnetars? Monthly Notices of the Royal Astronomical Society. ISSN 0035-8711

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Copyright, Publisher and Additional Information: © 2021 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Society. This is an author produced version of an article accepted for publication in Monthly Notices of the Royal Astronomical Society. Uploaded in accordance with the publisher's self-archiving policy.
Keywords: stars: neutron, magnetic fields, stars: massive, stars: magnetars, stars: magnetic field, methods: statistical
Dates:
  • Accepted: 19 April 2021
  • Published (online): 26 April 2021
Institution: The University of Leeds
Academic Units: The University of Leeds > Faculty of Engineering & Physical Sciences (Leeds) > School of Mathematics (Leeds) > Applied Mathematics (Leeds)
Depositing User: Symplectic Publications
Date Deposited: 29 Apr 2021 14:25
Last Modified: 29 Apr 2021 14:25
Status: Published online
Publisher: Oxford University Press
Identification Number: https://doi.org/10.1093/mnras/stab1175

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