Estimating the ages of eclipsing variable DM-stars on the basis of the evolutionary star models by Maeder and Meynet

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Scientific paper

A set of isochrones covering a wide range of star ages from 5\cdot106 to 1010 yr was built on the basis of the stellar models by A. Maeder and G. Meynet with overshooting and mass loss for Population I stars with abundances (X, Y, Z) = 0.70, 0.28, 0.02. The isochrones were used to compute the ages of 88 eclipsing variable stars from the catalog by Andersen which lie on the main sequence. The influence of initial data errors on the rezultes was investigated. The ages derived are in good agreement with the results of other authors.

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