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

Renzo, Mathieu; Gotberg, Ylva


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        <foaf:name>Renzo, Mathieu</foaf:name>
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        <foaf:name>Gotberg, Ylva</foaf:name>
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    <dct:title>Evolution of accretor stars in massive binaries: broader implications from modeling ζ Ophiuchi</dct:title>
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    <dct:issued rdf:datatype="http://www.w3.org/2001/XMLSchema#gYear">2021</dct:issued>
    <dcat:keyword>massive stars</dcat:keyword>
    <dcat:keyword>zeta ophiuchi</dcat:keyword>
    <dcat:keyword>binary</dcat:keyword>
    <dcat:keyword>Roche lobe overflow</dcat:keyword>
    <dcat:keyword>accretor</dcat:keyword>
    <dcat:keyword>runaway</dcat:keyword>
    <dct:issued rdf:datatype="http://www.w3.org/2001/XMLSchema#date">2021-04-19</dct:issued>
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    <dct:description>&lt;p&gt;Input and output files for MESA r15140 described in &lt;a href="https://ui.adsabs.harvard.edu/abs/2021arXiv210710933R/abstract"&gt;Renzo &amp;amp; Gotberg 2021&lt;/a&gt;. We used the MESA SDK x86_64-linux-20.12.1.&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 &lt;a href="https://github.com/mathren/zeta_oph"&gt;github&lt;/a&gt;.&lt;/p&gt;</dct:description>
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