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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 43.

Abundance profile of a CO WD (M = 0.611 ﹩{{\rm{M}}}_{\odot }﹩, ﹩{T}_{\mathrm{eff}}﹩ = 5.16 × ﹩{10}^{3}\;{\rm{K}}﹩, ﹩L=9.29\;\times \;{10}^{-5}\;{{\rm{L}}}_{\odot }﹩) after 4 Gyr of WD evolution. The region left of the blue, dashed line is the interior of the WD, where ﹩{\rm{\Gamma }}\geqslant 1﹩. Left of the red, dashed line ﹩{\rm{\Gamma }}\geqslant 50﹩, and diffusion has been turned off for this region. The electrons are an ideal gas to the right of the black dotted–dashed line.

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