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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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@dataset{meisel_zach_2019_2598716,
  author       = {Meisel, Zach},
  title        = {{Consistent Modeling of GS 1826-24 X-Ray Bursts for 
                   Multiple Accretion Rates Demonstrates the
                   Possibility of Constraining rp-process Reaction
                   Rates}},
  month        = mar,
  year         = 2019,
  publisher    = {Zenodo},
  version      = 9793,
  doi          = {10.5281/zenodo.2598716},
  url          = {https://doi.org/10.5281/zenodo.2598716}
}
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Publication date:
March 19, 2019
DOI:
10.5281/zenodo.2598716

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10.5281/zenodo.2598716

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Published in:
The Astrophysical Journal: Volume 860 pp. article id. 147, 7 pp. (2018) (Issue 2).
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Creative Commons Attribution 4.0 International

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Version 9793 10.5281/zenodo.2598716 Mar 19, 2019
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