期刊
ASTRONOMY & ASTROPHYSICS
卷 426, 期 1, 页码 L15-L18出版社
EDP SCIENCES S A
DOI: 10.1051/0004-6361:200400066
关键词
techniques : radial velocities; instrumentation : spectrographs; stars : planetary systems
We report the discovery of a transiting hot Jupiter around OGLE-TR-111, from our radial velocity follow-up of OGLE transiting candidates in Carina. The planet has a mass of 0.53 +/- 0.11 M-J and a radius of 1.0(-0.06)(+0.13) R-J. Three transiting exoplanets have already been found among OGLE candidates, all with periods near 1.5 days. The planet presented here, with P = 4.0 days, is the first exoplanet detected by transits with the characteristics of a normal hot Jupiter, as found in abundance by radial velocity surveys. The radius of OGLE-TR-111b and the scarcity of hot Jupiters detected among OGLE transit candidates tend to indicate that the case of HD 209458b, with a radius of 1.4 R-J, is exceptional, with most hot Jupiters being smaller.
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