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Testing models of accreting stars in massive binaries on ζ Ophiuchi

Renzo, Mathieu; Gotberg, Ylva


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  <identifier identifierType="DOI">10.5281/zenodo.4701565</identifier>
  <creators>
    <creator>
      <creatorName>Renzo, Mathieu</creatorName>
      <givenName>Mathieu</givenName>
      <familyName>Renzo</familyName>
      <nameIdentifier nameIdentifierScheme="ORCID" schemeURI="http://orcid.org/">0000-0002-6718-9472</nameIdentifier>
      <affiliation>Columbia University &amp; CCA</affiliation>
    </creator>
    <creator>
      <creatorName>Gotberg, Ylva</creatorName>
      <givenName>Ylva</givenName>
      <familyName>Gotberg</familyName>
      <nameIdentifier nameIdentifierScheme="ORCID" schemeURI="http://orcid.org/">0000-0002-6960-6911</nameIdentifier>
      <affiliation>Carnegie Observatories</affiliation>
    </creator>
  </creators>
  <titles>
    <title>Testing models of accreting stars in massive binaries on ζ Ophiuchi</title>
  </titles>
  <publisher>Zenodo</publisher>
  <publicationYear>2021</publicationYear>
  <subjects>
    <subject>massive stars</subject>
    <subject>zeta ophiuchi</subject>
    <subject>binary</subject>
    <subject>Roche lobe overflow</subject>
    <subject>accretor</subject>
    <subject>runaway</subject>
  </subjects>
  <dates>
    <date dateType="Issued">2021-04-19</date>
  </dates>
  <language>en</language>
  <resourceType resourceTypeGeneral="JournalArticle"/>
  <alternateIdentifiers>
    <alternateIdentifier alternateIdentifierType="url">https://zenodo.org/record/4701565</alternateIdentifier>
  </alternateIdentifiers>
  <relatedIdentifiers>
    <relatedIdentifier relatedIdentifierType="DOI" relationType="IsVersionOf">10.5281/zenodo.4701564</relatedIdentifier>
    <relatedIdentifier relatedIdentifierType="URL" relationType="IsPartOf">https://zenodo.org/communities/astronomy-general</relatedIdentifier>
    <relatedIdentifier relatedIdentifierType="URL" relationType="IsPartOf">https://zenodo.org/communities/mesa</relatedIdentifier>
  </relatedIdentifiers>
  <rightsList>
    <rights rightsURI="https://creativecommons.org/licenses/by/4.0/legalcode">Creative Commons Attribution 4.0 International</rights>
    <rights rightsURI="info:eu-repo/semantics/openAccess">Open Access</rights>
  </rightsList>
  <descriptions>
    <description descriptionType="Abstract">&lt;p&gt;Input and output files for MESA r15140 described in [https://ui.adsabs.harvard.edu/abs/2021arXiv210710933R/abstract](Renzo &amp;amp; Gotberg 2021).&lt;br&gt;
&lt;br&gt;
`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.&lt;br&gt;
&lt;br&gt;
`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.&lt;br&gt;
&lt;br&gt;
The other tarballs contain structures similar to `best_model.tar.gz` with parameter variations (see Sec. 6 and README.org).&lt;br&gt;
&lt;br&gt;
All parameter variations described in the paper can be obtained by modifying one (or more) parameters from the input files contained in these folders.&lt;br&gt;
&lt;br&gt;
A git repository for this project is available on [https://github.com/mathren90/zeta_oph](github).&lt;/p&gt;</description>
  </descriptions>
</resource>
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