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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="http://purl.org/dc/elements/1.1/" xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/oai_dc/ http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
  <dc:creator>Renzo, Mathieu</dc:creator>
  <dc:creator>Gotberg, Ylva</dc:creator>
  <dc:date>2021-04-19</dc:date>
  <dc:description>Input and output files for MESA r15140 described in [https://ui.adsabs.harvard.edu/abs/2021arXiv210710933R/abstract](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 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 [https://github.com/mathren90/zeta_oph](github).</dc:description>
  <dc:identifier>https://zenodo.org/record/4701565</dc:identifier>
  <dc:identifier>10.5281/zenodo.4701565</dc:identifier>
  <dc:identifier>oai:zenodo.org:4701565</dc:identifier>
  <dc:language>eng</dc:language>
  <dc:relation>doi:10.5281/zenodo.4701564</dc:relation>
  <dc:relation>url:https://zenodo.org/communities/astronomy-general</dc:relation>
  <dc:relation>url:https://zenodo.org/communities/mesa</dc:relation>
  <dc:rights>info:eu-repo/semantics/openAccess</dc:rights>
  <dc:rights>https://creativecommons.org/licenses/by/4.0/legalcode</dc:rights>
  <dc:subject>massive stars</dc:subject>
  <dc:subject>zeta ophiuchi</dc:subject>
  <dc:subject>binary</dc:subject>
  <dc:subject>Roche lobe overflow</dc:subject>
  <dc:subject>accretor</dc:subject>
  <dc:subject>runaway</dc:subject>
  <dc:title>Testing models of accreting stars in massive binaries on ζ Ophiuchi</dc:title>
  <dc:type>info:eu-repo/semantics/article</dc:type>
  <dc:type>publication-article</dc:type>
</oai_dc:dc>
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