A giant planet in the triple system HD 132563

@article{Desidera2011AGP,
  title={A giant planet in the triple system HD 132563},
  author={Silvano Desidera and Elena Carolo and Raffaele Gratton and A. F. Martinez Fiorenzano and Michael Endl and D. Mesa and Mauro Barbieri and Mariangela Bonavita and M. Cecconi and Riccardo Claudi and Rosario Cosentino and Francesco Marzari and Salvo Scuderi},
  journal={Astronomy and Astrophysics},
  year={2011},
  volume={533}
}
As part of our radial velocity planet-search survey performed with SARG at TNG, we monitored the components of HD 132563 for ten years. It is a binary system formed by two rather similar solar type stars with a projected separation of 4.1 arcsec, which corresponds to 400 AU at the distance of 96 pc. The two components are moderately metal-poor ([Fe/H]=–0.19), and the age of the system is about 5 Gyr. We detected RV variations of HD 132563B with period of 1544 days and semi-amplitude of 26 m/s… 
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