Astronomy and Astrophysics – Astrophysics
Scientific paper
Aug 2005
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005a%26a...439..367m&link_type=abstract
Astronomy and Astrophysics, Volume 439, Issue 1, August III 2005, pp.367-373
Astronomy and Astrophysics
Astrophysics
19
Stars: Individual: Hd 2638, Stars: Individual: Hd 27894, Hd 63454, Stars: Planetary Systems, Techniques: Radial Velocities, Techniques: Spectroscopic
Scientific paper
We report the discovery of three new planets, detected through Doppler measurements with the instrument harps installed on the ESO 3.6 m telescope, La Silla, Chile. These planets are orbiting the main-sequence stars HD 2638, HD 27894, and HD 63454. The orbital characteristics that best fit the observed data are depicted in this paper, as well as the stellar and planetary parameters. The planets' minimum mass is 0.48, 0.62, and 0.38 MJup for respectively HD 2638, HD 27894, and HD 63454; the orbital periods are 3.4442, 17.991, and 2.817822 days, corresponding to semi-major axis of 0.044, 0.122, and 0.036 AU, respectively. The observational data are carefully analysed for activity-induced effects and we conclude on the reliability of the observed radial-velocity variations as of exoplanetary origin. These three planets support the correlation between the star metallicity and the presence of planets (especially at short orbital distances), pointing towards the peculiar scenario of formation and migration of hot Jupiters.
Benz Willy
Bouchy Florent
Lo Curto Gaspare
Lovis Ch.
Mayor Marcel
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