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**Autoria(s):** TINGLEY, B.; ENDL, M.; GAZZANO, J. -C.; ALONSO, R.; MAZEH, T.; JORDA, L.; AIGRAIN, S.; ALMENARA, J. -M.; AUVERGNE, M.; BAGLIN, A.; BARGE, P.; BONOMO, A. S.; BORDE, P.; BOUCHY, F.; BRUNTT, H.; CABRERA, J.; CARPANO, S.; CARONE, L.; COCHRAN, W. D.; CSIZMADIA, Sz.; DELEUIL, M.; DEEG, H. J.; DVORAK, R.; ERIKSON, A.; FERRAZ-MELLO, S.; FRIDLUND, M.; GANDOLFI, D.; GILLON, M.; GUENTHER, E. W.; GUILLOT, T.; HATZES, A.; HEBRARD, G.; LEGER, A.; LLEBARIA, A.; LAMMER, H.; LOVIS, C.; MACQUEEN, P. J.; MOUTOU, C.; OLLIVIER, M.; OFIR, A.; PAETZOLD, M.; PEPE, F.; QUELOZ, D.; RAUER, H.; ROUAN, D.; SAMUEL, B.; SCHNEIDER, J.; SHPORER, A.; WUCHTERL, G.
Contribuinte(s)	UNIVERSIDADE DE SÃO PAULO
Data(s)	18/04/2012 18/04/2012 2011
Resumo	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 +/- 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 higher mass exoplanet orbits with a shorter period. Spanish Ministerio de Ciencia e Innovacion[ESP2007-65480-C02-02] Belgian Science Policy Office W. M. Keck Foundation NASA
Identificador	ASTRONOMY & ASTROPHYSICS, v.528, 2011 0004-6361 http://producao.usp.br/handle/BDPI/15622 10.1051/0004-6361/201015480 http://dx.doi.org/10.1051/0004-6361/201015480
Idioma(s)	eng
Publicador	EDP SCIENCES S A
Relação	Astronomy & Astrophysics
Direitos	closedAccess Copyright EDP SCIENCES S A
Palavras-Chave	#planetary systems #techniques: photometric #techniques: radial velocities #techniques: spectroscopic #ECHELLE SPECTROMETER #PLANETS #SATELLITES #PARAMETERS #EVOLUTION #SYSTEMS #Astronomy & Astrophysics
Tipo	article original article publishedVersion

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