Evolutionary status of UV Piscium and its comparison with other short period RS CVn binaries

Details Evolutionary status of UV Piscium and its comparison with other short period RS CVn binaries Evolutionary status of UV Piscium and its comparison with other short period RS CVn binaries

Aug 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005ap%26ss.298..461r&link_type=abstract

Astrophysics and Space Science, Volume 298, Issue 3, pp.461-468

Astronomy and Astrophysics

Astrophysics

1

Close Binaries, Eclipsing-Stars, Individual (Uv Piscium)-Stars, Late Type-Stars, Evolutionary Status

Scientific paper

From the derived elements of UV Piscium, the evolutionary status of both of its components are compared with the Schaller et al. models and also with other main sequence systems having spectral types of late F to K range. From these models the ages of the components of UV Psc are determined. The Rossby number, which is a measure of chromospheric activity, has been derived from the convective turnover time scales and also from the age estimates.

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