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Consistent Modeling of GS 1826-24 X-Ray Bursts for Multiple Accretion Rates Demonstrates the Possibility of Constraining rp-process Reaction Rates

Meisel, Zach


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  <dc:creator>Meisel, Zach</dc:creator>
  <dc:date>2019-03-19</dc:date>
  <dc:description>MESA inlists and run_star_extras associated with Meisel (2018). MESA version 9793.

Publication DOI: 10.3847/1538-4357/aac3d3</dc:description>
  <dc:identifier>https://zenodo.org/record/2598716</dc:identifier>
  <dc:identifier>10.5281/zenodo.2598716</dc:identifier>
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  <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>The Astrophysical Journal Volume 860(Issue 2) article id. 147, 7 pp. (2018)</dc:source>
  <dc:title>Consistent Modeling of GS 1826-24 X-Ray Bursts for Multiple Accretion Rates Demonstrates the Possibility of Constraining rp-process Reaction Rates</dc:title>
  <dc:type>info:eu-repo/semantics/other</dc:type>
  <dc:type>dataset</dc:type>
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