Astronomy and Astrophysics – Astrophysics
Scientific paper
2003-06-27
Astron.Astrophys.410:1051-1054,2003
Astronomy and Astrophysics
Astrophysics
4 pages, 2 figures, accepted for publication in A&A
Scientific paper
10.1051/0004-6361:20031341
We present radial-velocity measurements obtained with the ELODIE and AFOE spectrographs for GJ 777 A (HD 190360), a metal-rich ([Fe/H]=0.25) nearby (d=15.9 pc) star in a stellar binary system. A long-period low radial-velocity amplitude variation is detected revealing the presence of a Jovian planetary companion. Some of the orbital elements remain weakly constrained because of the smallness of the signal compared to our instrumental precision. The detailed orbital shape is therefore not well established. We present our best fitted orbital solution: an eccentric (e=0.48) 10.7--year orbit. The minimum mass of the companion is 1.33 M_Jup.
Beuzit Jean Luc
Brown Ted M.
Korzennik Sylvain G.
Mayor Marcel
Naef Dominique
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