Abstract
Models of α Cen A & B have been computed using the masses determined by Pourbaix et al. (2002) and the data derived from the spectroscopic analysis of Neuforge & Magain (1997). The seismological data obtained by Bouchy & Carrier (2001, 2002) do help improve our knowledge of the evolutionary status of the system. All the constraints are satisfied with a model which gives an age of about 6 Gyr for the binary.
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Thoul, A., Scuflaire, R., Noels, A., Vatovez, B., Briquet, M., Dupret, M. A., & Montalban, J. (2003). A new seismic analysis of alpha centauri. Astronomy and Astrophysics, 402(1), 293–297. https://doi.org/10.1051/0004-6361:20030244
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