A copy of this work was available on the public web and has been preserved in the Wayback Machine. The capture dates from 2018; you can also visit the original URL.
The file type is
Context. It seems that the recently identified class of pulsating stars, the γ Dor type-variables, includes objects with different metal abundances and a large percentage of binaries. Aims. We looked for indicators of metal abundance peculiarities and stellar binarity in a sample of 40 confirmed γ Dor stars. Methods. Absolute magnitudes from Hipparcos parallaxes and UV magnitudes, from the S2/S68 experiment on board the TD1 satellite, are retrieved from databases and compared with predicteddoi:10.1051/0004-6361:20065958 fatcat:spameqi5obeqvj2cgxpd6osiha