Figure 25 from MODULES FOR EXPERIMENTS IN STELLAR ASTROPHYSICS (MESA): BINARIES, PULSATIONS, AND EXPLOSIONS

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MODULES FOR EXPERIMENTS IN STELLAR ASTROPHYSICS (MESA): BINARIES, PULSATIONS, AND EXPLOSIONS

Authors: Bill Paxton, Pablo Marchant, Josiah Schwab, Evan B. Bauer, Lars Bildsten, Matteo Cantiello, Luc Dessart, R. Farmer, H. Hu, N. Langer, R. H. D. Townsend, Dean M. Townsley, and F. X. Timmes

2015 The Astrophysical Journal Supplement Series 220 15.

Provider: AAS Journals

Caption: Figure 25.

Radial velocity and ﹩{Y}_{{\rm{e}}}﹩ profiles at the onset of core collapse for the M_i = 15 ﹩{{\rm{M}}}_{\odot }﹩ model. Dashed curves show the results using a 22 isotope network and solid curves show the results using a 204 isotope network. Both models are evolved from the pre main-sequence to the onset of core collapse with their respective reaction network. The vertical gray lines mark the mass of the iron core as defined by the ﹩{Y}_{{\rm{e}}}﹩ jump.

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