The donor star radial velocity curve in the cataclysmic variable GY Cnc confirms white dwarf eclipse modelling mass

Littlefair, S.P. orcid.org/0000-0001-7221-855X, Rodríguez-Gil, P. orcid.org/0000-0002-4717-5102, Marsh, T.R. orcid.org/0000-0002-2498-7589 et al. (2 more authors) (2024) The donor star radial velocity curve in the cataclysmic variable GY Cnc confirms white dwarf eclipse modelling mass. Monthly Notices of the Royal Astronomical Society, 527 (2). pp. 4353-4358. ISSN 0035-8711

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Item Type: Article
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© The Author(s) 2023. Published by Oxford University Press on behalf of Royal Astronomical Society. This is an Open Access article distributed under the terms of the Creative Commons Attribution License (https://creativecommons.org/licenses/by/4.0/), which permits unrestricted reuse, distribution, and reproduction in any medium, provided the original work is properly cited.

Keywords: binaries: eclipsing; stars: dwarf novae; stars: evolution; novae, cataclysmic variables; white dwarfs.
Dates:
  • Published: January 2024
  • Published (online): 14 November 2023
  • Accepted: 8 November 2023
  • Submitted: 6 November 2023
Institution: The University of Sheffield
Academic Units: The University of Sheffield > Faculty of Science (Sheffield) > Department of Physics and Astronomy (Sheffield)
Funding Information:
Funder
Grant number
SCIENCE AND TECHNOLOGY FACILITIES COUNCIL
ST/V000853/1
Depositing User: Symplectic Sheffield
Date Deposited: 19 Jan 2024 12:05
Last Modified: 19 Jan 2024 12:05
Status: Published
Publisher: Oxford University Press (OUP)
Refereed: Yes
Identification Number: 10.1093/mnras/stad3500
Open Archives Initiative ID (OAI ID):

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