Meisel, Zach
2019-03-19
<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>
<p>Publication DOI: <a href="https://doi.org/10.3847/1538-4357/aac3d3">10.3847/1538-4357/aac3d3</a></p>
https://doi.org/10.5281/zenodo.2598716
oai:zenodo.org:2598716
Zenodo
https://doi.org/10.3847/1538-4357/aac3d3
https://zenodo.org/communities/mesa
https://doi.org/10.5281/zenodo.2598715
info:eu-repo/semantics/openAccess
Creative Commons Attribution 4.0 International
https://creativecommons.org/licenses/by/4.0/legalcode
The Astrophysical Journal, Volume 860(Issue 2), article id. 147, 7 pp. (2018), (2019-03-19)
Consistent Modeling of GS 1826-24 X-Ray Bursts for Multiple Accretion Rates Demonstrates the Possibility of Constraining rp-process Reaction Rates
info:eu-repo/semantics/other