Composite hot subdwarf binaries – I. The spectroscopically confirmed sdB sample

Vos, J., Németh, P., Vuc̆ković, M. et al. (2 more authors) (2018) Composite hot subdwarf binaries – I. The spectroscopically confirmed sdB sample. Monthly Notices of the Royal Astronomical Society, 473 (1). pp. 693-709. ISSN 0035-8711

Abstract

Metadata

Authors/Creators:
Copyright, Publisher and Additional Information: © 2017 The Author(s). Reproduced in accordance with the publisher's self-archiving policy.
Keywords: stars: abundances; binaries: spectroscopic; stars: fundamental parameters; stars: horizontal branch; stars: mass-loss; subdwarfs
Dates:
  • Published: 1 January 2018
  • Published (online): 24 October 2017
  • Accepted: 22 August 2017
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: 08 Dec 2017 13:07
Last Modified: 08 Dec 2017 13:07
Published Version: https://doi.org/10.1093/mnras/stx2198
Status: Published
Publisher: Oxford University Press
Refereed: Yes
Identification Number: https://doi.org/10.1093/mnras/stx2198

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