Doppler beaming factors for white dwarfs, main sequence stars, and giant stars. Limb-darkening coefficients for 3D (DA and DB) white dwarf models

Claret, A., Cukanovaite, E., Burdge, K. et al. (3 more authors) (2020) Doppler beaming factors for white dwarfs, main sequence stars, and giant stars. Limb-darkening coefficients for 3D (DA and DB) white dwarf models. Astronomy & Astrophysics, 641 (September 2020). A157. ISSN 0004-6361

Abstract

Metadata

Authors/Creators:
Copyright, Publisher and Additional Information: © ESO 2020. Reproduced in accordance with the publisher's self-archiving policy.
Keywords: stars: binaries: close; stars: evolution; stars: white dwarfs; stars: atmospheres; planetary systems
Dates:
  • Accepted: 27 July 2020
  • Published (online): 30 July 2020
  • Published: 24 September 2020
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/R003424/1
Depositing User: Symplectic Sheffield
Date Deposited: 26 Aug 2020 10:44
Last Modified: 24 Jan 2022 14:03
Status: Published
Publisher: EDP Sciences
Refereed: Yes
Identification Number: https://doi.org/10.1051/0004-6361/202038436
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