• Corpus ID: 117232062

Modeling of Alpha Cen and Procyon using VLTI observations

@article{Kervella2003ModelingOA,
  title={Modeling of Alpha Cen and Procyon using VLTI observations},
  author={Pierre Kervella and F. Th{\'e}venin and P. Morel and Gabrielle Berthomieu and Janine Provost and Pascal J. Bord{\'e} and Damien S{\'e}gransan},
  journal={arXiv: Astrophysics},
  year={2003}
}
We present a novel approach to model the nearby stars Alpha Cen A & B and Procyon A using asteroseismic and interferometric constraints. Using the VINCI instrument installed at the VLT Interferometer (VLTI), the angular diameters of the Alpha Centauri system were measured with a relative precision of 0.2% and 0.6%, respectively. From these values, we derive linear radii of R[A] = 1.224 +/- 0.003 R_sun and R[B] = 0.863 +/- 0.005 R_sun. These radii are in excellent agreement with the models of… 

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