Transiting exoplanets from the CoRoT space mission XV. CoRoT-15b: a brown-dwarf transiting companion
Contribuinte(s) |
UNIVERSIDADE DE SÃO PAULO |
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Data(s) |
18/04/2012
18/04/2012
2011
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Resumo |
We report the discovery by the CoRoT space mission of a transiting brown dwarf orbiting a F7V star with an orbital period of 3.06 days. CoRoT-15b has a radius of 1.12(-0.15)(+0.30) R(Jup) and a mass of 63.3 +/- 4.1 M(Jup), and is thus the second transiting companion lying in the theoretical mass domain of brown dwarfs. CoRoT-15b is either very young or inflated compared to standard evolution models, a situation similar to that of M-dwarf stars orbiting close to solar-type stars. Spectroscopic constraints and an analysis of the lightcurve imply a spin period in the range 2.9-3.1 days for the central star, which is compatible with a double-synchronisation of the system. Spanish Ministerio de Ciencia e Innovacion[ESP2007- 65480-C02-02] Deutsches Zentrum fur Luft- und Raumfahrt, DLR[50OW0204] Deutsches Zentrum fur Luft- und Raumfahrt, DLR[50OW0603] Deutsches Zentrum fur Luft- und Raumfahrt, DLR[50QP07011] Belgian Science Policy Office STFC[ST/G002266] |
Identificador |
ASTRONOMY & ASTROPHYSICS, v.525, 2011 0004-6361 http://producao.usp.br/handle/BDPI/15636 10.1051/0004-6361/201015276 |
Idioma(s) |
eng |
Publicador |
EDP SCIENCES S A |
Relação |
Astronomy & Astrophysics |
Direitos |
closedAccess Copyright EDP SCIENCES S A |
Palavras-Chave | #brown dwarfs #stars: low-mass #planetary systems #techniques: photometric #techniques: radial velocities #techniques: spectroscopic #EXTRASOLAR GIANT PLANETS #HYDROGEN-BURNING LIMIT #ECHELLE SPECTROMETER #CORALIE SURVEY #SOLAR PLANETS #RADIUS #STAR #MASS #PERIOD #EVOLUTION #Astronomy & Astrophysics |
Tipo |
article original article publishedVersion |