Figure 12 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 12.

s as a function of log₁₀ (ρ), for a 0.3 M_⊙, 10 Myr, α_MLT = 1.7 stellar model at Ω = 20 Ω_⊙, B_v-max = 10⁴ G, and δ = 0.03, including the rotating-only, magnetic-only, and unperturbed models. The rotating-only case is near-identical to the unperturbed model.

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