Evolution of massive AGB stars. III. (Siess, 2010)

Details Evolution of massive AGB stars. III. (Siess, 2010) Evolution of massive AGB stars. III. (Siess, 2010)

Jan 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010ycat..35129010s&link_type=abstract

VizieR On-line Data Catalog: J/A+A/512/A10. Originally published in: 2010A&A...512A..10S

Computer Science

1

Models: Evolutionary, Clusters: Globular

Scientific paper

The tables contains the stellar yields of 36 nuclei from H to 37Cl for 20 super-AGB stars of various initial masses between 7.5 and 10.5M&sun; and for metallicities ranging between Z=1e-4 and 0.04. The yields are given in solar mass and were computed using the postprocessing code considering the full coupling between the nuclear burning and the diffusive mixing. Table 2 provides the reference yields which do no experience third dredge-ups. Tables 3 and 4 simulate the effect of a high (lambda=0.8) and low (lambda=0.3) 3DUP efficiency. The intershell composition is set to 4He:12C:16O=0.66:0.31:0.02. Tables 5 and 6 simulate the yields which would result from an increase/decrease of the envelope temperature (Tenv) by+/-10%, respectively.
(5 data files).

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