Figure 27 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 27.

Mass fraction profiles of the ten most abundant isotopes within the iron core at the onset of core collapse for the M_i = 15 ﹩{{\rm{M}}}_{\odot }﹩ model evolved with the 204 isotope network. The entire iron core is in NSE and the mass fractions adapt to the changing temperature, density and ﹩{Y}_{{\rm{e}}}﹩.

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