期刊
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
卷 491, 期 2, 页码 1832-1850出版社
OXFORD UNIV PRESS
DOI: 10.1093/mnras/stz3154
关键词
Sun: abundances; stars: abundances; galaxy: abundances; galaxy: evolution
资金
- 'ChETEC' (Chemical Elements as Tracers of the Evolution of the Cosmos) COST Action of COST (European Cooperation in Science and Technology) [CA16117]
- European Founds for Regional Development (FEDER) [AYA2015-63588-P, PGC2018-095317-B-C21]
The decomposition of the Solar system abundances of heavy isotopes into their s- and r-components plays a key role in our understanding of the corresponding nuclear processes and the physics and evolution of their astrophysical sites. We present a new method for determining the s- and r-components of the Solar system abundances, fully consistent with our current understanding of stellar nucleosynthesis and galactic chemical evolution. The method is based on a study of the evolution of the solar neighbourhood with a state-of-the-art 1-zone model, using recent yields of low and intermediate mass stars as well as of massive rotating stars. We compare our results with previous studies and we provide tables with the isotopic and elemental contributions of the s- and r-processes to the Solar system composition.
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