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Testing models of accreting stars in massive binaries on ζ Ophiuchi

Renzo, Mathieu; Gotberg, Ylva

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<oai_dc:dc xmlns:dc="" xmlns:oai_dc="" xmlns:xsi="" xsi:schemaLocation="">
  <dc:creator>Renzo, Mathieu</dc:creator>
  <dc:creator>Gotberg, Ylva</dc:creator>
  <dc:description>Input and output files for MESA r15140 described in [](Renzo &amp; Gotberg 2021).

`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

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).</dc:description>
  <dc:subject>massive stars</dc:subject>
  <dc:subject>zeta ophiuchi</dc:subject>
  <dc:subject>Roche lobe overflow</dc:subject>
  <dc:title>Testing models of accreting stars in massive binaries on ζ Ophiuchi</dc:title>
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