On the Possibility of an Upper Limit on Magnetically Induced Radius Inflation in Low-mass Stars
The radii of low-mass stars are observed to be inflated above standard model predictions, especially in magnetically active stars. Typically, the empirical relative radius inflations Δ R / R are ≤10% but in (rare) cases may be ≥20%. Our magneto-convective stellar models have already replicated many...
| Published in: | The Astrophysical Journal |
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| Main Authors: | , |
| Format: | Article |
| Language: | English |
| Published: |
IOP Publishing
2024-01-01
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| Subjects: | |
| Online Access: | https://doi.org/10.3847/1538-4357/ad234e |