G. Doǧan, A. Bonanno, T. R. Bedding, T. L. Campante, J. Christensen-Dalsgaard, H. Kjeldsen
Abstract
We present our preliminary results of the modelling of the F5 star Procyon A. The frequencies predicted by our models are compared with the frequencies extracted through a global fit to the power spectrum obtained by the latest ground-based observations, which provides two different mode identification scenarios.
Keywords
stars: evolution - stars: individual (Procyon A) – stars: oscillations
Astronomische Nachrichten
Volume 331, Number 9-10, Page 949
2010 December
