Fig. 2.
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Original MESA and mapped models of the primary star. Shown are (a) density, (b) Mach number and (c) relative deviation from HSE according to Eq. (3) as a function of radius (quantities are averages over spherical shells). The times t = 447 d and t = 895 d correspond to the end of the damping and the end of the relaxation step, respectively. At time t = 0 d, there are no velocities in the AREPO model yet, and this is why the Mach number in panel b cannot be seen.
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