The secondary stars in cataclysmic variables and low-mass X-ray binaries

Smith, D.A. and Dhillon, V.S. orcid.org/0000-0003-4236-9642 (1998) The secondary stars in cataclysmic variables and low-mass X-ray binaries. Monthly Notices of the Royal Astronomical Society , 301 (3). pp. 767-781. ISSN 0035-8711

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Authors/Creators:
Copyright, Publisher and Additional Information: This article has been accepted for publication in [Journal Title] ©: 1998 RAS Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved.
Keywords: binaries : close; stars : late-type; novae, cataclysmic variables; X-rays : stars
Dates:
  • Published: 11 December 1998
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: 05 Oct 2017 15:36
Last Modified: 05 Oct 2017 15:36
Published Version: https://doi.org/10.1111/j.1365-8711.1998.02065.x
Status: Published
Publisher: Oxford University Press
Refereed: Yes
Identification Number: https://doi.org/10.1111/j.1365-8711.1998.02065.x

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