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A&A 392, L9-L12 (2002)
DOI: 10.1051/0004-6361:20021074
Letter
Asteroseismology and calibration of
Cen binary system
F. Thévenin1, J. Provost1, P. Morel1, G. Berthomieu1, F. Bouchy2 and F. Carrier2
1 Département Cassini, UMR CNRS 6529, Observatoire de la Côte d'Azur, BP 4229, 06304 Nice Cedex 4, France
2 Observatoire de Genève, 51 chemin des Maillettes, 1290 Sauverny, Switzerland
(Received 24 May (2002) / Accepted 22 July (2002) )
Abstract
Using the oscillation frequencies of
Cen A recently
discovered by Bouchy & Carrier (2001, (2002)),
the available astrometric, photometric and spectroscopic
data, we tried to improve the calibration of the
visual binary system
Cen.
With the revisited masses of Pourbaix et al. 2002
we did not succeed in obtaining a
solution satisfying all the seismic observational constraints.
Relaxing the constraints on the masses, we have found
an age
Myr,
an initial helium mass fraction
,
and an initial metallicity
,
with
and
for
Cen A & B.
Key words: stars: binaries: visual -- stars: evolution -- stars: oscillation -- stars: fundamental parameters -- stars: individual:
Offprint request: F. Thévenin, Frederic.Thevenin@obs-nice.fr
SIMBAD Objects
© ESO 2002
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