Figure 5 from Modules for Experiments in Stellar Astrophysics (MESA): Planets, Oscillations, Rotation, and Massive Stars

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Modules for Experiments in Stellar Astrophysics (MESA): Planets, Oscillations, Rotation, and Massive Stars

Authors: Bill Paxton, Matteo Cantiello, Phil Arras, Lars Bildsten, Edward F. Brown, Aaron Dotter, Christopher Mankovich, M. H. Montgomery, Dennis Stello, F. X. Timmes, and Richard Townsend

Paxton et al. 2013 The Astrophysical Journal Supplement Series 208 4.

Provider: AAS Journals

Caption: Figure 5.

Hertzsprung–Russell diagram and T _c–ρ _c evolution of a 1 M _☉ model evolving from pre-main sequence to the white dwarf cooling sequence. The number labels denote selected models, for which we show internal profiles in Figure 6.

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