Radius inflation in young low-mass stars follows a saturated Rossby-number relation like standard activity indicators, and depends directly on measured starspot covering fraction.
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The Relationship of Stellar Radius Inflation to Rotation and Magnetic Starspots at 10--670 Myr
Radius inflation in young low-mass stars follows a saturated Rossby-number relation like standard activity indicators, and depends directly on measured starspot covering fraction.