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Ultra-luminous X-ray sources and neutron-star-black-hole mergers from very massive close binaries at low metallicity

Marchant, Pablo; Langer, Norbert; Podsiadlowski, Philipp; Tauris, Thomas M.; de Mink, Selma; Mandel, Ilya; Moriya, Takashi J.


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  <identifier identifierType="DOI">10.5281/zenodo.3431313</identifier>
  <creators>
    <creator>
      <creatorName>Marchant, Pablo</creatorName>
      <givenName>Pablo</givenName>
      <familyName>Marchant</familyName>
      <nameIdentifier nameIdentifierScheme="ORCID" schemeURI="http://orcid.org/">0000-0002-0338-8181</nameIdentifier>
    </creator>
    <creator>
      <creatorName>Langer, Norbert</creatorName>
      <givenName>Norbert</givenName>
      <familyName>Langer</familyName>
    </creator>
    <creator>
      <creatorName>Podsiadlowski, Philipp</creatorName>
      <givenName>Philipp</givenName>
      <familyName>Podsiadlowski</familyName>
    </creator>
    <creator>
      <creatorName>Tauris, Thomas M.</creatorName>
      <givenName>Thomas M.</givenName>
      <familyName>Tauris</familyName>
    </creator>
    <creator>
      <creatorName>de Mink, Selma</creatorName>
      <givenName>Selma</givenName>
      <familyName>de Mink</familyName>
    </creator>
    <creator>
      <creatorName>Mandel, Ilya</creatorName>
      <givenName>Ilya</givenName>
      <familyName>Mandel</familyName>
    </creator>
    <creator>
      <creatorName>Moriya, Takashi J.</creatorName>
      <givenName>Takashi J.</givenName>
      <familyName>Moriya</familyName>
    </creator>
  </creators>
  <titles>
    <title>Ultra-luminous X-ray sources and neutron-star-black-hole mergers from very massive close binaries at low metallicity</title>
  </titles>
  <publisher>Zenodo</publisher>
  <publicationYear>2019</publicationYear>
  <dates>
    <date dateType="Issued">2019-03-19</date>
  </dates>
  <resourceType resourceTypeGeneral="Dataset"/>
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    <relatedIdentifier relatedIdentifierType="DOI" relationType="IsDocumentedBy">10.1051/0004-6361/201630188</relatedIdentifier>
    <relatedIdentifier relatedIdentifierType="DOI" relationType="IsVersionOf">10.5281/zenodo.2598794</relatedIdentifier>
    <relatedIdentifier relatedIdentifierType="URL" relationType="IsPartOf">https://zenodo.org/communities/mesa</relatedIdentifier>
  </relatedIdentifiers>
  <version>8845</version>
  <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;MESA inlists, run_star_extras, and data associated with&amp;nbsp;&lt;a href="https://ui.adsabs.harvard.edu/?#abs/2017A&amp;amp;A...604A..55M"&gt;Marchant et al. (2017)&lt;/a&gt;. MESA version 8118.&lt;/p&gt;

&lt;p&gt;Publication DOI:&amp;nbsp;&lt;a href="https://doi.org/10.1051/0004-6361/201630188"&gt;10.1051/0004-6361/201630188&lt;/a&gt;&lt;/p&gt;

&lt;p&gt;Files are also available in a gihub repository&amp;nbsp;&lt;a href="https://github.com/orlox/mesa_input_data/tree/master/2016_ULX"&gt;here&lt;/a&gt;&lt;/p&gt;

&lt;p&gt;Upload includes post-processed simulation output in the files Z-XX.tar.xz, where XX represents the metallicity (Z-25.tar.gz is for a metallicity of log10(Z)=-2.5). Each folder inside the archive corresponds to a single MESA simulation, with the name indicating the value of log10(M_1), q=M2/M1 and the orbital period in days. For example, the directory 1.600_0.500_0.900 corresponds to the simulation with log10(M1/Msun)=1.6, M2/M1=0.5 and Porb=0.9 days. Each folder is also a MESA template folder, containing all input files neccesary to reproduce that individual simulation.&lt;/p&gt;

&lt;p&gt;The file summary_tables.tar.gz contains summarized information for each simulation in ascii format.&lt;/p&gt;</description>
  </descriptions>
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