Ages of A-type Vega-like stars from uvby Photometry
arXiv:astro-ph/0010102 · doi:10.1086/318269
Abstract
We have estimated the ages of a sample of A-type Vega-like stars by using Strömgren \emph{uvby$β} photometric data and theoretical evolutionary tracks. We find that 13 percent of these A stars have been reported as Vega-like stars in the literature and that the ages of this subset run the gamut from very young (50~Myr) to old (1~Gyr), with no obvious age difference compared to those of field A stars. We clearly show that the fractional IR luminosity decreases with the ages of Vega-like stars.
4pages text, 3 tables, 3 figures, Accepted in ApJ
References in corpus (3)
Cited by in corpus (69)
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