Figure 13 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 13.

﹩{\mathrm{log}}_{10}({{\rm{\nabla }}}_{{\rm{s}}})﹩ as a function of log₁₀ (ρ), comparing S79 “rotating” models and our α_MLT(r) models (plus markers), for 0.3 M_⊙, (a) 10 Myr or (b) 1 Gyr, α_MLT = 1.7 stellar models at Ω = 5 − 20 Ω_⊙ (Δ5 Ω_⊙).

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