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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

MESA inlists and run_star_extras associated with Meisel (2018). MESA version 9793.

Publication DOI: 10.3847/1538-4357/aac3d3

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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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