Figure 9 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 9.

s as a function of log₁₀ (ρ), for 0.3 M_⊙, (a) 10 Myr or (b) 1 Gyr, α_MLT = 1.7 stellar models at some combinations of B_v-max = 10³–10⁵ G and (a) δ = 0.01–0.03 or (b) δ = 0.04–0.06, including the unperturbed model.

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