Figure 31 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 31.

Composition profiles of the eight most abundant isotopes at 1 s in the inner 0.4 ﹩{{\rm{M}}}_{\odot }﹩ of the ejecta for MESA (solid) and V1D (dashed) simulations of a 10⁵¹ erg explosion in the 15 ﹩{{\rm{M}}}_{\odot }﹩ model. The Si-rich and O-rich shells have been influenced by explosive nucleosynthesis, the former primarily for the production of ﹩{}^{56}\mathrm{Ni}﹩ and the latter primarily for the production of ﹩{}^{28}\mathrm{Si}﹩ and ﹩{}^{32}{\rm{S}}﹩.

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