March 19, 2019 Dataset Open Access

Marchant, Pablo; Langer, Norbert; Podsiadlowski, Philipp; Tauris, Thomas M.; Moriya, Takashi J.

DataCite XML Export

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  <identifier identifierType="DOI">10.5281/zenodo.2861541</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>Moriya, Takashi J.</creatorName>
      <givenName>Takashi J.</givenName>
      <familyName>Moriya</familyName>
    </creator>
  </creators>
  <titles>
    <title>A new route towards merging massive black holes</title>
  </titles>
  <publisher>Zenodo</publisher>
  <publicationYear>2019</publicationYear>
  <dates>
    <date dateType="Issued">2019-03-19</date>
  </dates>
  <resourceType resourceTypeGeneral="Dataset"/>
  <alternateIdentifiers>
    <alternateIdentifier alternateIdentifierType="url">https://zenodo.org/record/2861541</alternateIdentifier>
  </alternateIdentifiers>
  <relatedIdentifiers>
    <relatedIdentifier relatedIdentifierType="DOI" relationType="IsDocumentedBy">10.1051/0004-6361/201628133</relatedIdentifier>
    <relatedIdentifier relatedIdentifierType="DOI" relationType="IsVersionOf">10.5281/zenodo.2598750</relatedIdentifier>
    <relatedIdentifier relatedIdentifierType="URL" relationType="IsPartOf">https://zenodo.org/communities/mesa</relatedIdentifier>
  </relatedIdentifiers>
  <version>8118</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 &lt;a href="https://ui.adsabs.harvard.edu/?#abs/2016A&amp;amp;A...588A..50M"&gt;Marchant et al. (2016)&lt;/a&gt;. MESA version 8118.&lt;/p&gt;

&lt;p&gt;Publication DOI:&amp;nbsp;&lt;a href="https://doi.org/10.1051/0004-6361/201628133"&gt;10.1051/0004-6361/201628133&lt;/a&gt;&lt;/p&gt;

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

&lt;p&gt;Upload includes post-processed simulation output in the files Z04.tar.xz (for Z=Zsun/4), Z10.tar.xz&amp;nbsp;(for Z=Zsun/10),&amp;nbsp;Z20.tar.xz&amp;nbsp;(for Z=Zsun/20) and&amp;nbsp;Z50.tar.xz&amp;nbsp;(for Z=Zsun/50). Each folder inside the archive corresponds to a single MESA simulation, with the name indicating the value of log10(M_1), q=M2/M1&amp;nbsp;and the orbital period in days. For example, the directory 1.6_1.00_0.90 corresponds to the simulation with log10(M1)=1.6, M2/M1=1 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;</description>
  </descriptions>
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