CSIZMADIA, Szilard; HATZES, Artie P.; GANDOLFI, Davide; DELEUIL, Magali; BOUCHY, François; FRIDLUND, Malcolm C.; SZABADOS, L.; PARVIAINEN, H.; CABRERA, Juan; AIGRAIN, Suzanne; ALONSO, Roi; ALMENARA, J. M.; BAGLIN, Annie; BORDÉ, P.; BONOMO, Aldo Stefano; DEEG, Hans J.; DÍAZ, R. F.; ERIKSON, Anders; FERRAZ-MELLO, Sylvio; TADEU DOS SANTOS, M.; GUENTHER, Eike; GUILLOT, Tristan; GRZIWA, S.; HÉBRARD, Guillaume; KLAGYIVIK, P.; OLLIVIER, Marc; PÄTZOLD, M.; RAUER, Heike; ROUAN, Daniel; SANTERNE, A.; SCHNEIDER, Jean; MAZEH, Tsevi; WUCHTERL, Günther; CARPANO, Stefania; OFIR, Aviv

doi:10.1051/0004-6361/201526763

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CSIZMADIA, Szilard
Institute of Planetary Research, German Aerospace Center, Rutherfordstrasse 2, 12489, Berlin, Germany

HATZES, Artie P.
Türinger Landessternwarte Tautenburg

GANDOLFI, Davide
Università degli studi di Genova = University of Genoa [UniGe]

CSIZMADIA, Szilard
Institute of Planetary Research, German Aerospace Center, Rutherfordstrasse 2, 12489, Berlin, Germany

HATZES, Artie P.
Türinger Landessternwarte Tautenburg

GANDOLFI, Davide
Università degli studi di Genova = University of Genoa [UniGe]

DELEUIL, Magali
Laboratoire d'Astrophysique de Marseille [LAM]

BOUCHY, François
Laboratoire d'Astrophysique de Marseille [LAM]

FRIDLUND, Malcolm C.
Max-Planck-Institut für Astronomie [MPIA]

SZABADOS, L.
Konkoly Observatory of the Hungarian Academy of Sciences, MTA CSFK, Budapest, Konkoly Thege Miklos ut, 15-17, Hungary

PARVIAINEN, H.
Department of Physics

CABRERA, Juan
Institute of Planetary Research, German Aerospace Center, Rutherfordstrasse 2, 12489, Berlin, Germany

AIGRAIN, Suzanne
Department of Physics [Oxford]

ALONSO, Roi
Instituto de Astrofisica de Canarias [IAC]

ALMENARA, J. M.
Laboratoire d'Astrophysique de Marseille [LAM]

BAGLIN, Annie
Laboratoire d'études spatiales et d'instrumentation en astrophysique [LESIA]
Etoile
Haute résolution angulaire en astrophysique

BORDÉ, P.
Laboratoire d'Astrophysique de Bordeaux [Pessac] [LAB]

BONOMO, Aldo Stefano
INAF - Osservatorio Astrofisico di Torino [OATo]

DEEG, Hans J.
Instituto de Astrofisica de Canarias [IAC]

DÍAZ, R. F.
Observatoire Astronomique de l'Université de Genève [ObsGE]

ERIKSON, Anders
Institute of Planetary Research, German Aerospace Center, Rutherfordstrasse 2, 12489, Berlin, Germany

FERRAZ-MELLO, Sylvio
Instituto Astronômico e Geofísico, Universidade de São Paulo [IAG]

TADEU DOS SANTOS, M.
Instituto Astronômico e Geofísico, Universidade de São Paulo [IAG]

GUENTHER, Eike
Türinger Landessternwarte Tautenburg

GUILLOT, Tristan
Université Nice Sophia Antipolis (1965 - 2019) [UNS]

GRZIWA, S.
Rheinisches Institut für Umweltforschung [RIU]

HÉBRARD, Guillaume
Institut d'Astrophysique de Paris [IAP]

KLAGYIVIK, P.
Instituto de Astrofisica de Canarias [IAC]

OLLIVIER, Marc
Institut d'astrophysique spatiale [IAS]

PÄTZOLD, M.
Rheinisches Institut für Umweltforschung [RIU]

RAUER, Heike
Institute of Planetary Research, German Aerospace Center, Rutherfordstrasse 2, 12489, Berlin, Germany

ROUAN, Daniel
Laboratoire d'études spatiales et d'instrumentation en astrophysique [LESIA]
Etoile
Haute résolution angulaire en astrophysique

SANTERNE, A.
Universidade do Porto = University of Porto

SCHNEIDER, Jean
Laboratoire Univers et Théories [LUTH (UMR_8102)]

MAZEH, Tsevi
Tel Aviv University [TAU]

WUCHTERL, Günther
Türinger Landessternwarte Tautenburg

CARPANO, Stefania
Max Planck Institut für Plasma Physik and Excellence Cluster

OFIR, Aviv
Department of Earth and Planetary Sciences [Rehovot]

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Astronomy and Astrophysics - A&A. 2015, vol. 584, p. A131

EDP Sciences

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We report the detection of a rare transiting brown dwarf with a mass of 59 M<SUB>Jup</SUB> and radius of 1.1 R<SUB>Jup</SUB> around the metal-rich, [Fe/H] = 0.44, G9V star CoRoT-33. The orbit is eccentric (e = 0.07) with a period of 5.82 d. The companion, CoRoT-33b, is thus a new member in the so-called brown dwarf desert. The orbital period is within 3% to a 3:2 resonance with the rotational period of the star. CoRoT-33b may be an important test case for tidal evolution studies. The true frequency of brown dwarfs close to their host stars (P< 10 d) is estimated to be approximately 0.2% which is about six times smaller than the frequency of hot Jupiters in the same period range. We suspect that the frequency of brown dwarfs declines faster with decreasing period than that of giant planets.< Réduire

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Transiting exoplanets from the CoRoT space mission*. XXVIII. CoRoT-33b, an object in the brown dwarf desert with 2:3 commensurability with its host star

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