Published March 14, 2023
| Version v1
Dataset
Open
Supplemental Materials for "Convective boundary mixing in main-sequence stars: theory and empirical constraints"
Creators
- 1. Center for Interdisciplinary Exploration and Research in Astrophysics (CIERA), Northwestern University, 1800 Sherman Ave, Evanston, IL 60201,USA
- 2. Sydney Institute for Astronomy, School of Physics, University of Sydney NSW 2006, Australia
Description
MESA inlists and data products used for generating the figures of the review paper: "Convective boundary mixing in main-sequence stars: theory and empirical constraints".
Files
figure_1.zip
Files
(11.2 MB)
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md5:6cc675e25a8719e473073c859a9c55b1
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390.4 kB | Preview Download |
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md5:9261b7eb8731dccde68864c1bfee8b95
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3.7 kB | Preview Download |
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md5:3f806778f8cdc10510178e2be5b23ad1
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17.6 kB | Preview Download |
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md5:cdc0971626e4739f6a9f3e6ebac3b0d7
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26.7 kB | Preview Download |
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md5:dfd73978c0de564788f7bb1d02b9bd38
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4.4 MB | Preview Download |
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md5:1614e762170894ad493b499895ce292e
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5.5 kB | Preview Download |
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md5:5b74c598ff4a7b9a13cbea851164994c
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960.3 kB | Preview Download |
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md5:88aa6ec1cb450d1c8e3f82d5b2e85ea1
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5.4 MB | Preview Download |
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md5:86c74b6bfee97fdc1da2744e6486316d
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588 Bytes | Preview Download |
Additional details
Funding
- Kavli Institute for Theoretical Physics 1748958
- National Science Foundation