April 17, 2019 Dataset Open Access

Vigna-Gómez, Alejandro; Justham, Stephen; Mandel, Ilya; de Mink, Selma E.; Podsiadlowski, Philipp

DataCite XML Export

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  <identifier identifierType="DOI">10.5281/zenodo.2644593</identifier>
  <creators>
    <creator>
      <creatorName>Vigna-Gómez, Alejandro</creatorName>
      <givenName>Alejandro</givenName>
      <familyName>Vigna-Gómez</familyName>
      <nameIdentifier nameIdentifierScheme="ORCID" schemeURI="http://orcid.org/">0000-0003-1817-3586</nameIdentifier>
      <affiliation>University of Birmingham</affiliation>
    </creator>
    <creator>
      <creatorName>Justham, Stephen</creatorName>
      <givenName>Stephen</givenName>
      <familyName>Justham</familyName>
      <affiliation>University of Chinese Academy of Sciences</affiliation>
    </creator>
    <creator>
      <creatorName>Mandel, Ilya</creatorName>
      <givenName>Ilya</givenName>
      <familyName>Mandel</familyName>
      <nameIdentifier nameIdentifierScheme="ORCID" schemeURI="http://orcid.org/">0000-0002-6134-8946</nameIdentifier>
      <affiliation>Monash University</affiliation>
    </creator>
    <creator>
      <creatorName>de Mink, Selma E.</creatorName>
      <givenName>Selma E.</givenName>
      <familyName>de Mink</familyName>
      <nameIdentifier nameIdentifierScheme="ORCID" schemeURI="http://orcid.org/">0000-0001-9336-2825</nameIdentifier>
      <affiliation>University of Amsterdam</affiliation>
    </creator>
    <creator>
      <creatorName>Podsiadlowski, Philipp</creatorName>
      <givenName>Philipp</givenName>
      <familyName>Podsiadlowski</familyName>
      <nameIdentifier nameIdentifierScheme="ORCID" schemeURI="http://orcid.org/">0000-0002-8338-9677</nameIdentifier>
      <affiliation>Oxford University</affiliation>
    </creator>
  </creators>
  <titles>
    <title>Inlists for paper: Massive Stellar Mergers as Precursors of Hydrogen-rich Pulsational Pair Instability Supernovae</title>
  </titles>
  <publisher>Zenodo</publisher>
  <publicationYear>2019</publicationYear>
  <dates>
    <date dateType="Issued">2019-04-17</date>
  </dates>
  <resourceType resourceTypeGeneral="Dataset"/>
  <alternateIdentifiers>
    <alternateIdentifier alternateIdentifierType="url">https://zenodo.org/record/2644593</alternateIdentifier>
  </alternateIdentifiers>
  <relatedIdentifiers>
    <relatedIdentifier relatedIdentifierType="DOI" relationType="IsVersionOf">10.5281/zenodo.2644592</relatedIdentifier>
    <relatedIdentifier relatedIdentifierType="URL" relationType="IsPartOf">https://zenodo.org/communities/mesa</relatedIdentifier>
  </relatedIdentifiers>
  <version>1.0</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 (v10108) inlists for the models shown the &amp;quot;Massive Stellar Mergers as Precursors of Hydrogen-rich Pulsational Pair Instability Supernovae&amp;quot; Letter (1903.02135). The inlists reproduce both the single and merger model.&lt;/p&gt;

&lt;p&gt;Contents:&lt;/p&gt;

&lt;p&gt;FiducialMergersPPISN.tar.gz&lt;/p&gt;

&lt;ul&gt;
	&lt;li&gt;doubleMass&lt;/li&gt;
	&lt;li&gt;evolveMerged&lt;/li&gt;
	&lt;li&gt;evolveSingle&lt;/li&gt;
	&lt;li&gt;preMSmodel&lt;/li&gt;
	&lt;li&gt;README&lt;/li&gt;
&lt;/ul&gt;

&lt;p&gt;We also attach the single and merger MESA models at the moment where the central temperature is close to 10^9 K. These models where used to estimate the properties of the star, particularly core and envelope masses, as well as element abundances.&lt;/p&gt;

&lt;ul&gt;
	&lt;li&gt;mergerAtLogTc9.data&lt;/li&gt;
	&lt;li&gt;singleAtLogTc9.data&lt;/li&gt;
&lt;/ul&gt;</description>
  </descriptions>
</resource>