Galactic Evolution of Sr, Y, and Zr: A Multiplicity of Nucleosynthetic Processes
Max Planck Institute for Astrophysics · Osservatorio Astrofisico di Torino · +5 more institutions
Abstract
We follow the Galactic enrichment of three easily observed light n-capture elements Sr,Y,and Zr.Input stellar yields have been first separated into their respective main and weak s-process,and r-process components.The s-process yields from AGB stars are computed,exploring a wide range of efficiencies of the major neutron source,13C,and covering both disk and halo metallicities.AGBs have been shown to reproduce the main s-component in the solar system.The concurrent weak s-process,which accounts for the major fraction of the light s-process isotopes in the solar system and occurs in massive stars by the operation of the 22Ne n-source,is discussed in detail.Neither the main s-,nor the weak s-components are shown…
Citation impact
- FWCI
- 34.28
- Percentile
- 100%
- References
- 119
Authors
6- CTC. TravaglioCorresponding
Max Planck Institute for Astrophysics, Osservatorio Astrofisico di Torino, National Institute for Astrophysics
- RGR. Gallino
Istituto Nazionale di Fisica Nucleare, Sezione di Torino
- EAEnrico Arnone
The Open University, Istituto Nazionale di Fisica Nucleare, Sezione di Torino
- JJJ. J. Cowan
University of Oklahoma
- FJFaith Jordan
University of Oklahoma
Topics & keywords
- Physics
- Astrophysics
- s-process
- Metallicity
- Stars
- Nucleosynthesis
- Galactic halo
- Neutron capture