Figure 22 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 22.

Folded burst profiles for the different nuclear networks as compared to GS 1826-24 for an accretion rate of ﹩3\;\times \;{10}^{-9}\;{{\rm{M}}}_{\odot }\;{\mathrm{yr}}^{-1}﹩ with 2% metals with a solar composition, Three rp network models are shown and one of the adaptive net models. The insert shows a zoom in of the first ﹩30\;{\rm{s}}﹩ during the burst.

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