Low & intermediate mass stars chemical evolution (Gavilan+, 2005)

Details Low & intermediate mass stars chemical evolution (Gavilan+, 2005) Low & intermediate mass stars chemical evolution (Gavilan+, 2005)

Jan 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005ycat..34320861g&link_type=abstract

VizieR On-line Data Catalog: J/A+A/432/861. Originally published in: 2005A&A...432..861G

Computer Science

Models: Evolutionary, Abundances

Scientific paper

These tables show the complete content of Table 1 and Table 2 which give the production of elements in low and intermediate stars. Table 1 give the stellar yields for 5 values of metallicities: log(Z/Z{sun})=-0.2, -0.1, 0.0, +0.1 and +0.2, and for masses from 1 to 8M{sun}. Table 2 give the ejected mass by the stars during their evolution for the same metallicity range. This last one is the input file necessary to use in a chemical evolution model and it includes the stars up to 100M{sun}. The ejected masses for massive stars (m>8M{sun}) correspond to the production factors given by Woosley & Weaver (1995ApJS..101..181W).
(2 data files).

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