Asteroseismic modelling of Procyon A: Preliminary results
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, Page 949
December 2010
DOI: 10.1002/asna.201011433
ADS Bibliographic code: 2010arXiv1006.5912D