Published April 11, 2023
| Version v1
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Internal mixing of rotating stars inferred from dipole gravity modes
Creators
- 1. Institute of Astronomy, KU Leuven, Leuven, Belgium; Kavli Institute for Theoretical Physics, University of California, Santa Barbara, CA, USA
- 2. Institute of Astronomy, KU Leuven, Leuven, Belgium; Department of Astrophysics, IMAPP, Radboud University Nijmegen, Nijmegen, the Netherlands; Max Planck Institute for Astronomy, Heidelberg, Germany
- 3. Institute of Astronomy, KU Leuven, Leuven, Belgium
- 4. Department of Mathematics, Statistics and Physics, Newcastle University, Newcastle upon Tyne, UK; Planetary Science Institute, Tucson, AZ, USA
- 5. I-BioStat, Universiteit Hasselt, Hasselt, Belgium; I-BioStat, KU Leuven, Leuven, Belgium
Description
MESA and GYRE inlists, opacity tables, and supplementary material for the paper "Internal mixing of rotating stars inferred from dipole gravity modes" by Pedersen et al. (2021), Nature Astronomy, Volume 5, p. 715-722, DOI:10.1038/s41550-021-01351-x
Files
GYRE_setup.zip
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(127.4 MB)
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Additional details
Related works
- Is supplemented by
- Journal article: 10.1038/s41550-021-01351-x (DOI)