To be or not to be a black hole : detailed binary population models as a sanity check

Stevance, H.F., Parsons, S.G. orcid.org/0000-0002-2695-2654 and Eldridge, J.J. (2022) To be or not to be a black hole : detailed binary population models as a sanity check. Monthly Notices of the Royal Astronomical Society: Letters, 511 (1). L77-L81.

Abstract

Metadata

Authors/Creators:
Copyright, Publisher and Additional Information: © 2022 The Author(s). Reproduced in accordance with the publisher's self-archiving policy.
Keywords: stars: evolution; stars: black holes; (stars:) binaries: close; software: simulations
Dates:
  • Accepted: 8 January 2022
  • Published (online): 27 January 2022
  • Published: March 2022
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
Science and Technology Facilities CouncilST/R003424/1
Depositing User: Symplectic Sheffield
Date Deposited: 28 Jan 2022 12:39
Last Modified: 17 Nov 2022 15:34
Status: Published
Publisher: Oxford University Press (OUP)
Refereed: Yes
Identification Number: https://doi.org/10.1093/mnrasl/slac001
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