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A&A 460, 759-767 (2006)
DOI: 10.1051/0004-6361:20065251
Asteroseismology and evolutionary status of Procyon A
J. Provost1, G. Berthomieu1, M. Martic2, and P. Morel11 Département Cassiopée, UMR CNRS 6202, Observatoire de la Côte d'Azur, BP 4229, 06304 Nice Cedex 4, France
e-mail: janine.provost@obs-nice.fr
2 Service d'Aéronomie du CNRS, BP 3, 91371 Verrières-le-Buisson Cedex, France
(Received 22 March 2006 / Accepted 22 June 2006)
Abstract
Models of Procyon A satisfying the actual observational constraints,
particularly the asteroseismic ones, are discussed.
The oscillations of these models were computed and analysed.
We looked for seismic signatures of the evolutionary status of Procyon A.
We show that the behavior of the small frequency spacings,
particularly
allows us to distinguish
between main sequence and post-main sequence models,
all satisfying the observational
constraints on mass, effective temperature,
radius, and surface metallicity of Procyon A.
We also introduce a new seismic evolution criterion,
,
based on the comparison of the low and high frequency parts
of the power spectrum.
The comparison of the seismic properties of the models with
the available asteroseismic observations
does not allow us to
definitely decide on the stage of evolution of Procyon A.
Much more accurate frequencies must
be obtained especially in the low-frequency domain to distinguish between the models.
Key words: stars: oscillations -- stars: evolution -- stars: individual: Procyon A
© ESO 2006
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