The binary millisecond pulsar PSR J1023+0038 during its accretion state - I. Optical variability

Shahbaz, T., Linares, M., Nevado, S.P. et al. (7 more authors) (2015) The binary millisecond pulsar PSR J1023+0038 during its accretion state - I. Optical variability. Monthly Notices of the Royal Astronomical Society, 453 (4). pp. 3461-3473. ISSN 0035-8711

Abstract

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Authors/Creators:
Copyright, Publisher and Additional Information: This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society ©: 2015 The Author(s). Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved.
Keywords: binaries: close; stars: fundamental parameters; stars: individual: PSR J1023+0038; stars: neutron; X-rays: binaries
Dates:
  • Published: 9 September 2015
  • Accepted: 23 July 2015
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/J001589/1
SCIENCE AND TECHNOLOGY FACILITIES COUNCILST/M001350/1
Depositing User: Symplectic Sheffield
Date Deposited: 26 Oct 2017 14:05
Last Modified: 26 Oct 2017 14:06
Published Version: https://doi.org/10.1093/mnras/stv1686
Status: Published
Publisher: Oxford University Press
Refereed: Yes
Identification Number: https://doi.org/10.1093/mnras/stv1686
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