Figure 4 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 4.

Mass transfer rate and accretor radius as computed by MESA and STARS for an ﹩8\;{{\rm{M}}}_{\odot }+6.5\;{{\rm{M}}}_{\odot }﹩ binary with an initial orbital period of 3 days. All internal mixing processes (including convective mixing) are turned off in the calculations.

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