Stellar models until He burning - IV. (Claret+ 1998)

Details Stellar models until He burning - IV. (Claret+ 1998) Stellar models until He burning - IV. (Claret+ 1998)

Sep 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998ycat..41330123c&link_type=abstract

VizieR On-line Data Catalog: J/A+AS/133/123. Originally published in: 1998A&AS..133..123C

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Models: Evolutionary

Scientific paper

As a continuation of previous papers in a series devoted to the computation of stellar structure and evolution models we present a grid specifically obtained for detailed studies of the stellar content of the Small Magellanic Cloud. The initial metal content has thus been adopted to be Z=0.004 while the hydrogen content varies from 0.65 to 0.80 leaving as an intermediate value that given by standard laws of enrichment, X=0.744. Interpolation for different environment is therefore possible with these new models. Other input physics parameters, e.g. convective overshooting, mixing-length, opacities or nuclear reaction rates, have been adopted to be homogeneous with the previously published models in order to facilitate comparative studies. (1 data file).

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