Journal article Open Access

Evolution of accretor stars in massive binaries: broader implications from modeling ζ Ophiuchi

Renzo, Mathieu; Gotberg, Ylva


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{
  "publisher": "Zenodo", 
  "DOI": "10.5281/zenodo.4701565", 
  "language": "eng", 
  "title": "Evolution of accretor stars in massive binaries: broader implications from modeling \u03b6 Ophiuchi", 
  "issued": {
    "date-parts": [
      [
        2021, 
        4, 
        19
      ]
    ]
  }, 
  "abstract": "<p>Input and output files for MESA r15140 described in <a href=\"https://ui.adsabs.harvard.edu/abs/2021arXiv210710933R/abstract\">Renzo &amp; Gotberg 2021</a>. We used the MESA SDK x86_64-linux-20.12.1.<br>\n<br>\n`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.<br>\n<br>\n`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.<br>\n<br>\nThe other tarballs contain structures similar to `best_model.tar.gz` with parameter variations (see Sec. 6 and README.org).<br>\n<br>\nAll parameter variations described in the paper can be obtained by modifying one (or more) parameters from the input files contained in these folders.<br>\n<br>\nA git repository for this project is available on <a href=\"https://github.com/mathren/zeta_oph\">github</a>.</p>", 
  "author": [
    {
      "family": "Renzo, Mathieu"
    }, 
    {
      "family": "Gotberg, Ylva"
    }
  ], 
  "type": "article-journal", 
  "id": "4701565"
}
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