Doppler beaming factors for white dwarfs, main sequence stars, and giant stars Limb-darkening coefficients for 3D (DA and DB) white dwarf models (2020)
Attributed to:
Warwick Astronomy and Astrophysics Consolidated Grant 2017-2020
funded by
STFC
Abstract
No abstract provided
Bibliographic Information
Digital Object Identifier: http://dx.doi.org/10.1051/0004-6361/202038436
Publication URI: http://dx.doi.org/10.1051/0004-6361/202038436
Type: Journal Article/Review
Parent Publication: Astronomy & Astrophysics