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...
Saved in:
| Main Authors: | Lyra Cao, Keivan G. Stassun |
|---|---|
| Format: | Article |
| Language: | English |
| Published: |
IOP Publishing
2025-01-01
|
| Series: | The Astrophysical Journal Letters |
| Subjects: | |
| Online Access: | https://doi.org/10.3847/2041-8213/ade875 |
| Tags: |
Add Tag
No Tags, Be the first to tag this record!
|
Similar Items
-
Starspot Area Coverage: Correlation with Age and Spectral Type in FGK and M Stars
by: Alexandre Araújo, et al.
Published: (2025-01-01) -
Starspots as an Explanation for the Mysterious IYJ Continuum Excess Emission in Classical T Tauri Stars
by: Facundo Pérez Paolino, et al.
Published: (2024-01-01) -
Precise Parameters from Bayesian Spectral Energy Distribution Fitting Indicate Thermally Driven Mass Loss Likely Driver of Radius Valley
by: David Jordan, et al.
Published: (2025-01-01) -
Testing the Rossby Paradigm: Weakened Magnetic Braking in Early K-type Stars
by: Travis S. Metcalfe, et al.
Published: (2025-01-01) -
Flares on TRAPPIST-1 Reveal the Spectrum of Magnetic Features on Its Surface
by: Valeriy Vasilyev, et al.
Published: (2025-01-01)