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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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{
  "publisher": "Zenodo", 
  "DOI": "10.5281/zenodo.2598716", 
  "container_title": "The Astrophysical Journal", 
  "title": "Consistent Modeling of GS 1826-24 X-Ray Bursts for Multiple Accretion Rates Demonstrates the Possibility of Constraining rp-process Reaction Rates", 
  "issued": {
    "date-parts": [
      [
        2019, 
        3, 
        19
      ]
    ]
  }, 
  "abstract": "<p>MESA inlists and run_star_extras associated with <a href=\"https://ui.adsabs.harvard.edu/#abs/2018arXiv180505552M/abstract\">Meisel (2018)</a>. MESA version 9793.</p>\n\n<p>Publication DOI:&nbsp;<a href=\"https://doi.org/10.3847/1538-4357/aac3d3\">10.3847/1538-4357/aac3d3</a></p>", 
  "author": [
    {
      "family": "Meisel, Zach"
    }
  ], 
  "page": "article id. 147, 7 pp. (2018)", 
  "volume": "Volume 860", 
  "version": "9793", 
  "type": "dataset", 
  "issue": "Issue 2", 
  "id": "2598716"
}
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March 19, 2019
DOI:
10.5281/zenodo.2598716

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The Astrophysical Journal: Volume 860 pp. article id. 147, 7 pp. (2018) (Issue 2).
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Version 9793 10.5281/zenodo.2598716 Mar 19, 2019
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