The CORALIE survey for southern extra-solar planets - X. A Hot Jupiter orbiting HD73256

被引:40
作者
Udry, S
Mayor, M
Clausen, JV
Freyhammer, LM
Helt, BE
Lovis, C
Naef, D
Olsen, EH
Pepe, F
Queloz, D
Santos, NC
机构
[1] Observ Geneva, CH-1290 Sauverny, Switzerland
[2] Niels Bohr Inst Astron Phys & Geophys, DK-2100 Copenhagen O, Denmark
[3] Astron Observ, DK-2100 Copenhagen O, Denmark
[4] Royal Observ Belgium, B-1180 Brussels, Belgium
[5] Free Univ Brussels, B-1050 Brussels, Belgium
[6] Univ Lisbon, Ctr Astron & Astrophys, Observ Astron Lisboa, P-1349018 Lisbon, Portugal
关键词
techniques : radial velocities; techniques : photometric; stars : binaries : spectroscopic; stars : individual : HD 73256; stars : activity; stars : planetary systems;
D O I
10.1051/0004-6361:20030815
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Recent radial-velocity measurements obtained with the CORALIE spectrograph on the 1.2-m Euler Swiss telescope at La Silla unveil the presence of a new Jovian-mass Hot Jupiter around HD73256. The 1.85-M-Jup planet moves on an extremely short-period (P = 2.5486 d), quasi-circular orbit. The best Keplerian orbital solution is presented together with an unsuccessful photometric planetary-transit search performed with the SAT Danish telescope at La Silla. Over the time span of the observations, the photometric follow-up of the candidate has nevertheless revealed a P similar or equal to 14-d photometric periodicity corresponding to the rotational period of the star. This variation as well as the radial-velocity jitter around the Keplerian solution are shown to be related to the fair activity level known for HD73256.
引用
收藏
页码:679 / 684
页数:6
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