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Fig. 3
Radius inflation due to irradiation. Δlog R is plotted against ΔL/L0 for masses ℳ = 0.2(0.1)0.6 ℳ⊙. Here ΔL is the increment in Lr within the convective envelope and L0 is the ZAMS luminosity for mass ℳ. For clarity, consecutive curves are displaced vertically by 0.015.
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