The Relationship of Stellar Radius Inflation to Rotation and Magnetic Starspots at 10–670 Myr
Active, low-mass stars are widely observed to have radii that are larger than predicted by standard stellar models. Proposed mechanisms for this radius inflation generally involve stellar magnetism, either in the form of added pressure support in the outer layers or suppression of convection via sta...
保存先:
| 主要な著者: | , |
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| フォーマット: | Artigo |
| 言語: | Inglês |
| 出版事項: |
IOP Publishing
2025-01-01
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| シリーズ: | The Astrophysical Journal Letters |
| 主題: | |
| オンライン･アクセス: | https://doi.org/10.3847/2041-8213/ade875 |
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