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A&A 467, 1389-1396 (2007)
DOI: 10.1051/0004-6361:20066641
New grids of stellar models including tidal-evolution constants up to carbon burning
IV. From 0.8 to 125
: high metallicities (Z = 0.04-0.10)
A. Claret Instituto de Astrofísica de Andalucía, CSIC, Apartado 3004, 18080 Granada, Spain
e-mail: claret@iaa.es
(Received 26 October 2006 / Accepted 28 January 2007)
Abstract
Aims.The aim of the present grid of stellar models
is to complete our previous calculations and provide a
tool for investigating the astrophysical properties of eclipsing
binaries, stellar clusters, galactic bulges, and elliptical
galaxies with a high metal content.
Methods.To explore the applicability of high metallic models,
we have computed three grids: (X,
Z) = (0.64, 0.04),
(0.58, 0.06), and (0.46, 0.10). For all these grids, we
adopted an enrichment law
, as in
our previous papers on this subject. The input physics is almost
the same as adopted in our earlier work except for some numerical details,
recent measurement of the rate for the reaction
14N(
)15O, and the recent mass-loss rate for the Wolf-Rayet
stages.
Results.Two high-metallicity clusters, NGC 6253 and NGC 6791, were used to test the present
calculations with very satisfactory results.
On the other hand, as this series of grids was mainly designed to investigate
the tidal evolution of close binaries, we analyse the present status
of circularization times in both clusters and
isolated binaries. The present models (90 tables) can be retrieved from the
CDS via anonymous ftp.
Key words: binaries: eclipsing -- stars: evolution -- stars: abundances -- stars: rotation
© ESO 2007
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