Poster abstract details

In this paper we present a grid of stellar models (for $0.8M_{\odot} - 6M_{\odot}$, $Z=0.01-0.04$) obtained with CESAM2k stellar evolutionary code. We determined also the corresponding seismic properties using the LNAWENR/ROMOSC linear, non-adiabatic, non-radial stellar pulsation code.