Relative Contributions of the Weak, Main, and Fission-recycling r-process

doi:10.3847/0004-637X/816/2/79

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@ARTICLE{2016ApJ...816...79S,
 author = {{Shibagaki}, S. and {Kajino}, T. and {Mathews}, G.~J. and {Chiba}, S. and {Nishimura}, S. and {Lorusso}, G.},
 title = "{Relative Contributions of the Weak, Main, and Fission-recycling r-process}",
 journal = {\apj},
 keywords = {nuclear reactions, nucleosynthesis, abundances, stars: abundances, supernovae: general, Astrophysics - Solar and Stellar Astrophysics, Astrophysics - High Energy Astrophysical Phenomena, Nuclear Theory},
 year = 2016,
 month = jan,
 volume = {816},
 number = {2},
 eid = {79},
 pages = {79},
 doi = {10.3847/0004-637X/816/2/79},
archivePrefix = {arXiv},
 eprint = {1505.02257},
 primaryClass = {astro-ph.SR},
 adsurl = {https://ui.adsabs.harvard.edu/abs/2016ApJ...816...79S},
 adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

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