Published October 1, 2016 | Version v1
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Models of low-mass helium white dwarfs including gravitational settling, thermal and chemical diffusion, and rotational mixing⋆

Description

MESA inlists, data (from a single run: rotation + diffusion, M1=1.4, M2=1.2, Porb=3.4 days, Z=0.02) and run_star_extras  associated with Istrate et. al 2016. MESA version 7624.  The grid of models produced in this paper can be found here.

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