Evolution of accretor stars in massive binaries: broader implications from modeling ζ Ophiuchi
Description
Input and output files for MESA r15140 described in Renzo & Gotberg 2021. We used the MESA SDK x86_64-linux-20.12.1.
`fiducial.tar.xz` contains the MESA work directories and output for the evolution of the model described in Sec. 3, one for the evolution in a binary, and one after detachment to finish the main sequence of the accreting star.
`single_stars.tar.xz` contains rotating single star models labeled according to their initial mass, and for each mass non-rotating (no-rot) and rotating models (labelled based on the initial omega/omega_crit) are provided.
The other tarballs contain structures similar to `best_model.tar.gz` with parameter variations (see Sec. 6 and README.org).
All parameter variations described in the paper can be obtained by modifying one (or more) parameters from the input files contained in these folders.
A git repository for this project is available on github.
Files
composition_accretor.mp4
Files
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