Published February 7, 2024
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Probability distributions of initial rotation velocities and core-boundary mixing efficiencies of γ Doradus stars
Authors/Creators
Contributors
Researcher (2):
-
1.
KU Leuven
- 2. Katholieke Universiteit Leuven
- 3. Universiteit Hasselt
Description
MESA setup for models of rotating gamma Doradus stars, as described in Mombarg, Aerts & Molenberghs (2024, A&A). The text file contains a shear profile computed the ESTER code (see Mombarg et al. 2022, ApJ, 925, 154) that is used for the computation of rotational mixing.
Files
r-dOmega_dr_profile_M3.0Xc0.95_O20.txt
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(149.9 kB)
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Additional details
Funding
- Agence Nationale de la Recherche
- MASSIF ANR-21-CE31-0018-02
- KU Leuven
- PARADISE C16/18/005
- European Research Council
- 4D-STAR 101071505
Dates
- Accepted
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2024-02-07