Dataset Open Access
Vigna-Gómez, Alejandro;
Justham, Stephen;
Mandel, Ilya;
de Mink, Selma E.;
Podsiadlowski, Philipp
<?xml version='1.0' encoding='utf-8'?> <oai_dc:dc xmlns:dc="http://purl.org/dc/elements/1.1/" xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/oai_dc/ http://www.openarchives.org/OAI/2.0/oai_dc.xsd"> <dc:creator>Vigna-Gómez, Alejandro</dc:creator> <dc:creator>Justham, Stephen</dc:creator> <dc:creator>Mandel, Ilya</dc:creator> <dc:creator>de Mink, Selma E.</dc:creator> <dc:creator>Podsiadlowski, Philipp</dc:creator> <dc:date>2019-04-17</dc:date> <dc:description>MESA (v10108) inlists for the models shown the "Massive Stellar Mergers as Precursors of Hydrogen-rich Pulsational Pair Instability Supernovae" Letter (1903.02135). The inlists reproduce both the single and merger model. Contents: FiducialMergersPPISN.tar.gz doubleMass evolveMerged evolveSingle preMSmodel README 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. mergerAtLogTc9.data singleAtLogTc9.data </dc:description> <dc:identifier>https://zenodo.org/record/2644593</dc:identifier> <dc:identifier>10.5281/zenodo.2644593</dc:identifier> <dc:identifier>oai:zenodo.org:2644593</dc:identifier> <dc:relation>doi:10.5281/zenodo.2644592</dc:relation> <dc:relation>url:https://zenodo.org/communities/mesa</dc:relation> <dc:rights>info:eu-repo/semantics/openAccess</dc:rights> <dc:rights>https://creativecommons.org/licenses/by/4.0/legalcode</dc:rights> <dc:title>Inlists for paper: Massive Stellar Mergers as Precursors of Hydrogen-rich Pulsational Pair Instability Supernovae</dc:title> <dc:type>info:eu-repo/semantics/other</dc:type> <dc:type>dataset</dc:type> </oai_dc:dc>
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