S-process in low-mass extremely metal-poor stars

Details S-process in low-mass extremely metal-poor stars S-process in low-mass extremely metal-poor stars

Feb 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012epjwc..1902009c&link_type=abstract

Assembling the Puzzle of the Milky Way, Le Grand-Bornand, France, Edited by C. Reylé; A. Robin; M. Schultheis; EPJ Web of Confer

Physics

Scientific paper

We present post-processing s-process calculations for the core He-flash of a 1M&sun; star with and Z = 10-8. Our model shows neutron densities larger than 1014cm-3, resulting in the production of s-process elements. The model reproduces the C, O, Sr, and Ba abundances of the star hyper metal-poor star HE0107-5240 within a factor of 4.

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