Figure 4 from The Radius and Entropy of a Magnetized, Rotating, Fully Convective Star: Analysis with Depth-dependent Mixing Length Theories

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The Radius and Entropy of a Magnetized, Rotating, Fully Convective Star: Analysis with Depth-dependent Mixing Length Theories

Authors: Lewis G. Ireland, and Matthew K. Browning

2018 The Astrophysical Journal 856 132.

Provider: AAS Journals

Caption: Figure 4.

The ratio of stellar radii R₂/R₁ as a function Δs_ad via Equation (18), for 0.3 M_⊙, (a) 10 Myr or (b) 1 Gyr stellar models at α_MLT = 0.5–1.7 (Δ0.05). We see a divergence at 1 Gyr, which arise from deviations from the ideal equation of state. y = x (orange) is plotted for ease of comparison.

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