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The Relationship of Stellar Radius Inflation to Rotation and Magnetic Starspots at 10–670 Myr

  • Authors: Lyra Cao, Keivan G. Stassun

Lyra Cao and Keivan G. Stassun 2025 The Astrophysical Journal Letters 988 .

  • Provider: AAS Journals

Caption: Figure B1.

Markov Chain Monte Carlo corner plots showing parameters recovered for the power-law fit in Figure 2. The best-fit values are, for rotational saturation: ﹩\mathrm{log}{{\rm{Ro}}}_{{\rm{crit}}}=-1.39{6}_{-0.070}^{+0.076}﹩; spot saturation level: ﹩{f}_{\mathrm{spot},\mathrm{sat}}=0.27{6}_{-0.016}^{+0.017}﹩; slope at ﹩\mathrm{log}{\rm{Ro}}\gt \mathrm{log}{{\rm{Ro}}}_{{\rm{crit}}}﹩: ﹩{m}_{{\rm{slope}}}=1.15{4}_{-0.081}^{+0.087}﹩.

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