Transiting exoplanets from the CoRoT space mission: XIII. CoRoT-14b: an unusually dense very hot Jupiter

In this paper, the CoRoT Exoplanet Science Team announces its 14th discovery. Herein, we discuss the observations and analyses that allowed us to derive the parameters of this system: a hot Jupiter with a mass of $7.6 \pm 0.6$ Jupiter masses orbiting a solar-type star (F9V) with a period of only 1.5...

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Λεπτομέρειες βιβλιογραφικής εγγραφής
Κύριοι συγγραφείς: Tingley, B, Endl, M, Gazzano, J, Alonso, R, Mazeh, T, Jorda, L, Aigrain, S, Almenara, J, Auvergne, M, Baglin, A, Barge, P, Bonomo, A, Bordé, P, Bouchy, F, Bruntt, H, Cabrera, J, Carpano, S, Carone, L, Cochran, W, Csizmadia, S, Deleuil, M, Deeg, H, Dvorak, R, Erikson, A, Ferraz-Mello, S
Μορφή: Journal article
Γλώσσα:English
Έκδοση: 2011
Περιγραφή
Περίληψη:In this paper, the CoRoT Exoplanet Science Team announces its 14th discovery. Herein, we discuss the observations and analyses that allowed us to derive the parameters of this system: a hot Jupiter with a mass of $7.6 \pm 0.6$ Jupiter masses orbiting a solar-type star (F9V) with a period of only 1.5 d, less than 5 stellar radii from its parent star. It is unusual for such a massive planet to have such a small orbit: only one other known exoplanet with a higher mass orbits with a shorter period.