Talk abstract details

We present our preliminary results of modelling the F5
star Procyon A, including the comparison between the two different
evolutionary codes that have been employed: ASTEC (Aarhus STellar
Evolution Code) (Christensen-Dalsgaard, 2008b) and GARSTEC (Garching
Stellar Evolution Code) (Weiss & Schlattl, 2008). Aarhus adiabatic
pulsation package (ADIPLS) (Christensen-Dalsgaard, 2008a) has been
used to calculate the frequencies of the models. Our modelling is
compared to the preliminary frequency analysis of ground based
observations which suggests two different mode identification
scenarios.