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Up: Grids of stellar

4. How to obtain the tables electronically

The following data is available for each model:

tex2html_wrap_inline1243, tex2html_wrap_inline1245, tex2html_wrap_inline1247, tex2html_wrap_inline1249, tex2html_wrap_inline1251, tex2html_wrap_inline1253, tex2html_wrap_inline1255, tex2html_wrap_inline1257, tex2html_wrap_inline1259, tex2html_wrap_inline1261, tex2html_wrap_inline1263, tex2html_wrap_inline1265, tex2html_wrap_inline1267, tex2html_wrap_inline1269, tex2html_wrap_inline1271, tex2html_wrap_inline1155, tex2html_wrap_inline1153, tex2html_wrap_inline1277, tex2html_wrap_inline1279, tex2html_wrap_inline1281, tex2html_wrap_inline1283, tex2html_wrap_inline1285, tex2html_wrap_inline1287, tex2html_wrap_inline1289, tex2html_wrap_inline1291, tex2html_wrap_inline1293, tex2html_wrap_inline1295

where tex2html_wrap_inline1297 and tex2html_wrap_inline1299 are the abundances, in mass fractions, at the surface and at the center of the star, respectively, tex2html_wrap_inline1267 the convective core mass fraction (overshooting included), tex2html_wrap_inline1269 the uncorrected value of tex2html_wrap_inline1305 (for WR stars only),

and tex2html_wrap_inline1171 and tex2html_wrap_inline1173 the central density and temperature, respectively. More detailed descriptions of the model selection and the table contents are given in Paper I.

These data, as well as the ones relative to the previous published grids (Papers I to VI), are accessible electronically at the Centre de Données Stellaires de Strasbourg (CDS, see A&A 1992, Vol. 266 No. 2, page E1, or at http://cdsweb.u-strasbg.fr/CDS.html). The data can also be obtained from the Geneva Observatory by means of anonymous ftp at obsftp.unige.ch in the directory pub/evol/modelz100, or through the Web at http://obswww.unige.ch.

Acknowledgements

We thank Drs. D.R. Alexander and J.W. Ferguson for providing us with the low temperature opacity tables.



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