Properties of OB star-black hole systems derived from detailed binary evolution models

Langer, N., Schürmann, C., Stoll, K. et al. (38 more authors) (2020) Properties of OB star-black hole systems derived from detailed binary evolution models. Astronomy and Astrophysics. ISSN 0004-6361

Abstract

Metadata

Authors/Creators:
  • Langer, N.
  • Schürmann, C.
  • Stoll, K.
  • Marchant, P.
  • Lennon, D.J.
  • Mahy, L.
  • Mink, S.E.D.
  • Quast, M.
  • Riedel, W.
  • Sana, H.
  • Schneider, P.
  • Schootemeijer, A.
  • Wang, C.
  • Almeida, L.A.
  • Bestenlehner, J.M. https://orcid.org/0000-0002-0859-5139
  • Bodensteiner, J.
  • Castro, N.
  • Clark, S.
  • Crowther, P.A.
  • Dufton, P.
  • Evans, C.J.
  • Fossati, L.
  • Gräfener, G.
  • Grassitelli, L.
  • Grin, N.
  • Hastings, B.
  • Herrero, A.
  • Koter, A.D.
  • Menon, A.
  • Patrick, L.
  • Puls, J.
  • Renzo, M.
  • Sander, A.A.C.
  • Schneider, F.R.N.
  • Sen, K.
  • Shenar, T.
  • Simón-Días, S.
  • Tauris, T.M.
  • Tramper, F.
  • Vink, J.S.
  • Xu, X.-T.
Copyright, Publisher and Additional Information: © ESO 2020. Reproduced in accordance with the publisher's self-archiving policy.
Keywords: astro-ph.SR; astro-ph.SR; astro-ph.HE; stars: massive – stars; early-type – stars; Wolf-Rayet – stars; interiors – stars; rotation – stars; evolution
Dates:
  • Accepted: 9 April 2020
  • Published (online): 20 April 2020
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: 20 May 2020 12:16
Last Modified: 20 May 2020 12:16
Status: Published online
Publisher: EDP Sciences
Refereed: Yes
Identification Number: https://doi.org/10.1051/0004-6361/201937375
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