4.6 Article

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

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ASTRONOMY & ASTROPHYSICS
卷 407, 期 2, 页码 679-684

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E D P SCIENCES
DOI: 10.1051/0004-6361:20030815

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techniques : radial velocities; techniques : photometric; stars : binaries : spectroscopic; stars : individual : HD 73256; stars : activity; stars : planetary systems

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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.

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