Issue |
A&A
Volume 584, December 2015
|
|
---|---|---|
Article Number | A13 | |
Number of page(s) | 12 | |
Section | Planets and planetary systems | |
DOI | https://doi.org/10.1051/0004-6361/201526763 | |
Published online | 13 November 2015 |
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
1
Institute of Planetary Research, German Aerospace Center,
Rutherfordstrasse
2,
12489
Berlin,
Germany
e-mail:
szilard.csizmadia@dlr.de
2
Thüringer Landessternwarte, Sternwarte 5, Tautenburg
5, 07778
Tautenburg,
Germany
3
Dipartimento di Fisica, Universitá di Torino,
via P. Giuria 1, 10125
Torino,
Italy
4
Landessternwarte Königstuhl, Zentrum für Astronomie der
Universität Heidelberg, Königstuhl
12, 69117
Heidelberg,
Germany
5
Aix Marseille Université, CNRS, LAM (Laboratoire d’Astrophysique
de Marseille) UMR 7326, 13388
Marseille,
France
6
Max-Planck-Institut für Astronomie, Königstuhl 17, 69117
Heidelberg,
Germany
7
Leiden Observatory, University of Leiden,
PO Box 9513, 2300 RA, Leiden, The Netherlands
8
Department of Earth and Space Sciences, Chalmers University of
Technology, Onsala Space Observatory, 439 92
Onsala,
Sweden
9
Konkoly Observatory of the Hungarian Academy of
Sciences, MTA CSFK,
Budapest, Konkoly Thege Miklós
út
15-17,
Hungary
10
Sub-department of Astrophysics, Department of Physics, University
of Oxford, Oxford,
OX1 3RH,
UK
11
Department of Physics, Denys Wilkinson Building, Keble Road,
Oxford, OX1 3RH, UK
12
Instituto de Astrofísica de Canarias, 38205, La Laguna, Tenerife, Spain
13
Universidad de La Laguna, Dept. de Astrofísica, 38206,
La Laguna, Tenerife,
Spain
14
LESIA, UMR 8109 CNRS, Observatoire de Paris, UPMC, Université
Paris-Diderot, 5 place J.
Janssen, 92195
Meudon,
France
15
LAB, UMR 5804, Univ. Bordeaux & CNRS,
33270
Floirac,
France
16 INAF–Osservatorio Astrofisico di Torino Strada
Osservatorio, 20 10025 Pino Torinese ( TO), Italy
17
Observatoire astronomique de l’Université de Genève,
51 ch. des Maillettes,
1290
Versoix,
Switzerland
18 IAG-Universidade de São Paulo, 1226 Sâo Paulo, Brasil
19
Université de Nice-Sophia Antipolis, CNRS UMR 6202, Observatoire
de la Côte d’Azur, BP
4229, 06304
Nice Cedex 4,
France
20
Rheinisches Institut für Umweltforschung an der Universität zu
Köln, 50931
Aachener Strasse 209,
Germany
21
Institut d’Astrophysique de Paris, UMR 7095 CNRS, Université
Pierre & Marie Curie, 98bis
boulevard Arago, 75014
Paris,
France
22
Institut d’Astrophysique Spatiale, Université Paris
XI, 91405
Orsay,
France
23
Center for Astronomy and Astrophysics, TU Berlin, Hardenbergstr.
36, 10623
Berlin,
Germany
24
Instituto de Astrofísica e Ciências do Espaço, Universidade do
Porto, CAUP, Rua das
Estrelas, 4150-762
Porto,
Portugal
25
LUTH, Observatoire de Paris, UMR 8102 CNRS, Université Paris
Diderot, 5 place Jules
Janssen, 92195
Meudon,
France
26
School of Physics and Astronomy, Raymond and Beverly Sackler
Faculty of Exact Sciences, 39040 Tel Aviv University, Tel Aviv, Israel
27
Max-Planck-Institut für extraterrestrische Physik,
Giessenbachstrasse 1,
85748
Garching,
Germany
28
Department of Earth and Planetary Sciences, Weizmann Institute of
Science, 234 Herzl
St., 76100
Rehovot,
Israel
Received: 16 June 2015
Accepted: 28 July 2015
We report the detection of a rare transiting brown dwarf with a mass of 59 MJup and radius of 1.1 RJup 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.
Key words: brown dwarfs / stars: rotation / eclipses
The CoRoT space mission, launched on December 27th 2006, has been developed and is operated by CNES, with the contribution of Austria, Belgium, Brazil, ESA (RSSD and Science Programme), Germany and Spain. Based on observations made with HARPS (High Accuracy Radial velocity Planet Searcher) spectrograph on the 3.6-m European Organisation for Astronomical Research in the Southern Hemisphere telescope at La Silla Observatory, Chile (ESO program 188.C-0779).
Based on observations obtained with the Nordic Optical Telescope, operated on the island of La Palma jointly by Denmark, Finland, Iceland, Norway, and Sweden, in the Spanish Observatorio del Roque de los Muchachos of the Instituto de Astrofisica de Canarias, in time allocated by the Spanish Time Allocation Committee (CAT).
© ESO, 2015
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.