Origin of Stellar Abundances in the early Galaxy

Details Origin of Stellar Abundances in the early Galaxy Origin of Stellar Abundances in the early Galaxy

Oct 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aipc..947..364m&link_type=abstract

VII LATIN AMERICAN SYMPOSIUM ON NUCLEAR PHYSICS AND APPLICATIONS. AIP Conference Proceedings, Volume 947, pp. 364-370 (2007).

Other

Hydrostatic Stellar Nucleosynthesis, Nucleosynthesis In Novae, Supernovae, And Other Explosive Environments, Neutron Stars

Scientific paper

Observations of metal-poor stars in the last decade have revealed an abundance pattern that have recently been explained as the result of two nucleosynthesis processes, a strong r-process that creates most of the Z>=56 and some 38<=Z<=47 abundances and a light element primary process (LEPP) responsible for creating the remaining 38<=Z<=47 abundances and some small contribution to heavier elements. We review some of the current literature on the LEPP and show a derived abundance pattern as a function of mass number.

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