articleThe Astrophysical JournalFeb 1, 2004BRONZE OA

Galactic Evolution of Sr, Y, and Zr: A Multiplicity of Nucleosynthetic Processes

Max Planck Institute for Astrophysics · Osservatorio Astrofisico di Torino · +5 more institutions

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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…

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