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Constructing stable 3D hydrodynamical models of giant stars

Ohlmann, Sebastian T.; Röpke, Friedrich K.; Pakmor, Rüdiger; Springel, Volker


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  <dc:creator>Ohlmann, Sebastian T.</dc:creator>
  <dc:creator>Röpke, Friedrich K.</dc:creator>
  <dc:creator>Pakmor, Rüdiger</dc:creator>
  <dc:creator>Springel, Volker</dc:creator>
  <dc:date>2019-03-19</dc:date>
  <dc:description>MESA inlist associated with Ohlmann et al. (2017). MESA version 6208.

Publication DOI: 10.1051/0004-6361/201629692</dc:description>
  <dc:identifier>https://zenodo.org/record/2598737</dc:identifier>
  <dc:identifier>10.5281/zenodo.2598737</dc:identifier>
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  <dc:relation>doi:10.1051/0004-6361/201629692</dc:relation>
  <dc:relation>doi:10.5281/zenodo.2598736</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:source>Astronomy &amp; Astrophysics Volume 599 id.A5, 16 pp. (2017)</dc:source>
  <dc:title>Constructing stable 3D hydrodynamical models of giant stars</dc:title>
  <dc:type>info:eu-repo/semantics/other</dc:type>
  <dc:type>dataset</dc:type>
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