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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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  "description": "<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>", 
  "license": "https://creativecommons.org/licenses/by/4.0/legalcode", 
  "creator": [
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      "@type": "Person", 
      "name": "Meisel, Zach"
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  "url": "https://zenodo.org/record/2598716", 
  "datePublished": "2019-03-19", 
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  "identifier": "https://doi.org/10.5281/zenodo.2598716", 
  "@id": "https://doi.org/10.5281/zenodo.2598716", 
  "@type": "Dataset", 
  "name": "Consistent Modeling of GS 1826-24 X-Ray Bursts for Multiple Accretion Rates Demonstrates the Possibility of Constraining rp-process Reaction Rates"
}
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