Abundances of Fe and Sr in the metal-poor stars. NLTE analysis with 1D and <3D> model atmospheres

Details Abundances of Fe and Sr in the metal-poor stars. NLTE analysis with 1D and <3D> model atmospheres Abundances of Fe and Sr in the metal-poor stars. NLTE analysis with 1D and <3D> model atmospheres

Jan 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012cemw.confe..13b&link_type=article

The Chemical Evolution of the Milky Way, held January 23 - 27, 2012 at the Sexten Center for Astrophysics (SCfA). Sesto Pusteria

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