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Transiting exoplanets from the CoRoT space mission VI. CoRoT-Exo-3b : the first secure inhabitant of the brown-dwarf desert

Identifieur interne : 002F13 ( PascalFrancis/Curation ); précédent : 002F12; suivant : 002F14

Transiting exoplanets from the CoRoT space mission VI. CoRoT-Exo-3b : the first secure inhabitant of the brown-dwarf desert

Auteurs : M. Deleuil [France] ; H. J. Deeg [Espagne] ; R. Alonso [France] ; F. Bouchy [France] ; D. Rouan [France] ; M. Auvergne [France] ; A. Baglin [France] ; S. Aigrain [Royaume-Uni] ; J. M. Almenara [Espagne] ; M. Barbieri [France] ; P. Barge [France] ; H. Bruntt [Australie] ; P. Bordd [France] ; A. Collier Cameron [Royaume-Uni] ; Sz. Csizmadia [Allemagne] ; R. De La Reza [Brésil] ; R. Dvorak [Autriche] ; A. Erikson [Allemagne] ; M. Fridlund [Pays-Bas] ; D. Gandolfi [Allemagne] ; M. Gillon [Suisse] ; E. Guenther [Allemagne] ; T. Guillot [France] ; A. Hatzes [Allemagne] ; G. Hebrard [France] ; L. Jorda [France] ; H. Lammer [Autriche] ; A. Leger [France] ; A. Llebaria [France] ; B. Loeillet [France] ; M. Mayor [Suisse] ; T. Mazeh [Israël] ; C. Moutou [France] ; M. Ollivier [France] ; M. P Tzold [Allemagne] ; F. Pont [Royaume-Uni] ; D. Queloz [Suisse] ; H. Rauer [Allemagne] ; J. Schneider [France] ; A. Shporer [Israël] ; G. Wuchterl [Allemagne] ; S. Zucker [Israël]

Source :

RBID : Pascal:09-0016503

Descripteurs français

English descriptors

Abstract

Context. The CoRoT space mission routinely provides high-precision photometric measurements of thousands of stars that have been continuously observed for months. Aims. The discovery and characterization of the first very massive transiting planetary companion with a short orbital period is reported. Methods. A series of 34 transits was detected in the CoRoT light curve of an F3V star, observed from May to October 2007 for 152 days. The radius was accurately determined and the mass derived for this new transiting, thanks to the combined analysis of the light curve and complementary ground-based observations: high-precision radial-velocity measurements, on-off photometry, and high signal-to-noise spectroscopic observations. Results. CoRoT-Exo-3b has a radius of 1.01 ± 0.07 RJup and transits around its F3-type primary every 4.26 days in a synchronous orbit. Its mass of 21.66 ± 1.0MJup, density of 26.4 ±5.6 g cm-3, and surface gravity of log g = 4.72 clearly distinguish it from the regular close-in planet population, making it the most intriguing transiting substellar object discovered so far. Conclusions. With the current data, the nature of CoRoT-Exo-3b is ambiguous, as it could either be a low-mass brown-dwarf or a member of a new class of "superplanets". Its discovery may help constrain the evolution of close-in planets and brown-dwarfs better. Finally, CoRoT-Exo-3b confirms the trend that massive transiting giant planets (M > 4 MJup) are found preferentially around more massive stars than the Sun.
pA  
A01 01  1    @0 0004-6361
A02 01      @0 AAEJAF
A03   1    @0 Astron. astrophys. : (Berl., Print)
A05       @2 491
A06       @2 3
A08 01  1  ENG  @1 Transiting exoplanets from the CoRoT space mission VI. CoRoT-Exo-3b : the first secure inhabitant of the brown-dwarf desert
A11 01  1    @1 DELEUIL (M.)
A11 02  1    @1 DEEG (H. J.)
A11 03  1    @1 ALONSO (R.)
A11 04  1    @1 BOUCHY (F.)
A11 05  1    @1 ROUAN (D.)
A11 06  1    @1 AUVERGNE (M.)
A11 07  1    @1 BAGLIN (A.)
A11 08  1    @1 AIGRAIN (S.)
A11 09  1    @1 ALMENARA (J. M.)
A11 10  1    @1 BARBIERI (M.)
A11 11  1    @1 BARGE (P.)
A11 12  1    @1 BRUNTT (H.)
A11 13  1    @1 BORDD (P.)
A11 14  1    @1 COLLIER CAMERON (A.)
A11 15  1    @1 CSIZMADIA (Sz.)
A11 16  1    @1 DE LA REZA (R.)
A11 17  1    @1 DVORAK (R.)
A11 18  1    @1 ERIKSON (A.)
A11 19  1    @1 FRIDLUND (M.)
A11 20  1    @1 GANDOLFI (D.)
A11 21  1    @1 GILLON (M.)
A11 22  1    @1 GUENTHER (E.)
A11 23  1    @1 GUILLOT (T.)
A11 24  1    @1 HATZES (A.)
A11 25  1    @1 HEBRARD (G.)
A11 26  1    @1 JORDA (L.)
A11 27  1    @1 LAMMER (H.)
A11 28  1    @1 LEGER (A.)
A11 29  1    @1 LLEBARIA (A.)
A11 30  1    @1 LOEILLET (B.)
A11 31  1    @1 MAYOR (M.)
A11 32  1    @1 MAZEH (T.)
A11 33  1    @1 MOUTOU (C.)
A11 34  1    @1 OLLIVIER (M.)
A11 35  1    @1 PÄTZOLD (M.)
A11 36  1    @1 PONT (F.)
A11 37  1    @1 QUELOZ (D.)
A11 38  1    @1 RAUER (H.)
A11 39  1    @1 SCHNEIDER (J.)
A11 40  1    @1 SHPORER (A.)
A11 41  1    @1 WUCHTERL (G.)
A11 42  1    @1 ZUCKER (S.)
A14 01      @1 Laboratoire d'Astrophysique de Marseille (UMR 6110), Technopole de Marseille-Étoile @2 13388 Marseille @3 FRA @Z 1 aut. @Z 3 aut. @Z 10 aut. @Z 11 aut. @Z 26 aut. @Z 29 aut. @Z 30 aut. @Z 33 aut.
A14 02      @1 Instituto de Astrofísica de Canarias, C. via Lactea S/N @2 38200 La Laguna @3 ESP @Z 2 aut. @Z 9 aut.
A14 03      @1 Institut d'Astrophysique de Paris, UMR7095 CNRS, Université Pierre & Marie Curie, 98bis Bd Arago @2 75014 Paris @3 FRA @Z 4 aut. @Z 25 aut. @Z 30 aut.
A14 04      @1 LESIA, CNRS UMR 8109, Observatoire de Paris, 5 place J. Janssen @2 92195 Meudon @3 FRA @Z 5 aut. @Z 6 aut. @Z 7 aut.
A14 05      @1 School of Physics, University of Exeter, Stocker Road @2 Exeter EX4 4QL @3 GBR @Z 8 aut. @Z 36 aut.
A14 06      @1 School of Physics A28, University of Sydney @3 AUS @Z 12 aut.
A14 07      @1 IAS, Université Paris XI @2 91405 Orsay @3 FRA @Z 13 aut. @Z 28 aut. @Z 34 aut.
A14 08      @1 School of Physics and Astronomy, University of St Andrews @3 GBR @Z 14 aut.
A14 09      @1 Institute of Planetary Research, DLR, Rutherfordstr. 2 @2 12489 Berlin @3 DEU @Z 15 aut. @Z 18 aut. @Z 38 aut.
A14 10      @1 Observatório Nacional @2 Rio de Janeiro, RJ @3 BRA @Z 16 aut.
A14 11      @1 Institute for Astronomy, University of Vienna, Tûrkenschanzstrasse 17 @2 1180 Vienna @3 AUT @Z 17 aut.
A14 12      @1 Research and Scientific Support Department, European Space Agency, ESTEC @2 2200 Noordwijk @3 NLD @Z 19 aut.
A14 13      @1 Thüringer Landesstemwarte Tautenburg, Sternwarte 5 @2 07778 Tautenburg @3 DEU @Z 20 aut. @Z 22 aut. @Z 24 aut. @Z 41 aut.
A14 14      @1 Observatoire de Genève, Université de Genève, 51 Ch. des Maillettes @2 1290 Sauverny @3 CHE @Z 21 aut. @Z 31 aut. @Z 37 aut.
A14 15      @1 Observatoire de la Côte d'Azur, Laboratoire Cassiopée, CNRS UMR 6202, BP 4229 @2 06304 Nice @3 FRA @Z 23 aut.
A14 16      @1 Space Research Institute, Austrian Academy of Sciences, Schmiedlstrasse 6 @2 8042 Graz @3 AUT @Z 27 aut.
A14 17      @1 School of Physics and Astronomy, R. and B. Sackler Faculty of Exact Sciences, Tel Aviv University @2 Tel Aviv 69978 @3 ISR @Z 32 aut. @Z 40 aut. @Z 42 aut.
A14 18      @1 Rheinisches Institut für Umweltforschung, Universität zu Kôln, Abt. Planetenforschung, Aachener Str. 209 @2 50931 Kôln @3 DEU @Z 35 aut.
A14 19      @1 Center for Astronomy and Astrophysics, TU Berlin, Hardenbergstr. 36 @2 10623 Berlin @3 DEU @Z 38 aut.
A14 20      @1 LUTH, Observatoire de Paris-Meudon, 5 place J. Janssen @2 92195 Meudon @3 FRA @Z 39 aut.
A20       @1 889-897
A21       @1 2008
A23 01      @0 ENG
A43 01      @1 INIST @2 14176 @5 354000183994860280
A44       @0 0000 @1 © 2009 INIST-CNRS. All rights reserved.
A45       @0 1/2 p.
A47 01  1    @0 09-0016503
A60       @1 P
A61       @0 A
A64 01  1    @0 Astronomy and astrophysics : (Berlin. Print)
A66 01      @0 FRA
C01 01    ENG  @0 Context. The CoRoT space mission routinely provides high-precision photometric measurements of thousands of stars that have been continuously observed for months. Aims. The discovery and characterization of the first very massive transiting planetary companion with a short orbital period is reported. Methods. A series of 34 transits was detected in the CoRoT light curve of an F3V star, observed from May to October 2007 for 152 days. The radius was accurately determined and the mass derived for this new transiting, thanks to the combined analysis of the light curve and complementary ground-based observations: high-precision radial-velocity measurements, on-off photometry, and high signal-to-noise spectroscopic observations. Results. CoRoT-Exo-3b has a radius of 1.01 ± 0.07 RJup and transits around its F3-type primary every 4.26 days in a synchronous orbit. Its mass of 21.66 ± 1.0MJup, density of 26.4 ±5.6 g cm-3, and surface gravity of log g = 4.72 clearly distinguish it from the regular close-in planet population, making it the most intriguing transiting substellar object discovered so far. Conclusions. With the current data, the nature of CoRoT-Exo-3b is ambiguous, as it could either be a low-mass brown-dwarf or a member of a new class of "superplanets". Its discovery may help constrain the evolution of close-in planets and brown-dwarfs better. Finally, CoRoT-Exo-3b confirms the trend that massive transiting giant planets (M > 4 MJup) are found preferentially around more massive stars than the Sun.
C02 01  3    @0 001E03
C03 01  3  FRE  @0 Planète extrasolaire @5 26
C03 01  3  ENG  @0 Extrasolar planets @5 26
C03 02  3  FRE  @0 Naine brune @5 27
C03 02  3  ENG  @0 Brown dwarf stars @5 27
C03 03  3  FRE  @0 Courbe lumière @5 28
C03 03  3  ENG  @0 Light curves @5 28
C03 04  3  FRE  @0 Vitesse radiale @5 29
C03 04  3  ENG  @0 Radial velocity @5 29
C03 05  3  FRE  @0 Photométrie @5 30
C03 05  3  ENG  @0 Photometry @5 30
C03 06  X  FRE  @0 Observation spectroscopique @5 31
C03 06  X  ENG  @0 Spectroscopical observation @5 31
C03 06  X  SPA  @0 Observación espectroscópica @5 31
C03 07  3  FRE  @0 Orbite @5 32
C03 07  3  ENG  @0 Orbits @5 32
C03 08  3  FRE  @0 Gravité surface @5 33
C03 08  3  ENG  @0 Surface gravity @5 33
C03 09  X  FRE  @0 Planète géante @5 34
C03 09  X  ENG  @0 Giant planet @5 34
C03 09  X  SPA  @0 Planeta gigante @5 34
C03 10  3  FRE  @0 Etoile massive @5 35
C03 10  3  ENG  @0 Massive stars @5 35
C03 11  3  FRE  @0 Soleil @5 36
C03 11  3  ENG  @0 Sun @5 36
C03 12  X  FRE  @0 Système planétaire @5 37
C03 12  X  ENG  @0 Planetary system @5 37
C03 12  X  SPA  @0 Sistema planetario @5 37
C03 13  3  FRE  @0 Etoile faible masse @5 38
C03 13  3  ENG  @0 Low-mass stars @5 38
N21       @1 007
N44 01      @1 OTO
N82       @1 OTO

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Pascal:09-0016503

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<name sortKey="Baglin, A" sort="Baglin, A" uniqKey="Baglin A" first="A." last="Baglin">A. Baglin</name>
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<name sortKey="Aigrain, S" sort="Aigrain, S" uniqKey="Aigrain S" first="S." last="Aigrain">S. Aigrain</name>
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<s1>School of Physics, University of Exeter, Stocker Road</s1>
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<name sortKey="Almenara, J M" sort="Almenara, J M" uniqKey="Almenara J" first="J. M." last="Almenara">J. M. Almenara</name>
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<name sortKey="Barbieri, M" sort="Barbieri, M" uniqKey="Barbieri M" first="M." last="Barbieri">M. Barbieri</name>
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<name sortKey="Barge, P" sort="Barge, P" uniqKey="Barge P" first="P." last="Barge">P. Barge</name>
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<name sortKey="Collier Cameron, A" sort="Collier Cameron, A" uniqKey="Collier Cameron A" first="A." last="Collier Cameron">A. Collier Cameron</name>
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<s1>School of Physics and Astronomy, University of St Andrews</s1>
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<name sortKey="Csizmadia, Sz" sort="Csizmadia, Sz" uniqKey="Csizmadia S" first="Sz." last="Csizmadia">Sz. Csizmadia</name>
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<s1>Institute of Planetary Research, DLR, Rutherfordstr. 2</s1>
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<country>Allemagne</country>
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<name sortKey="De La Reza, R" sort="De La Reza, R" uniqKey="De La Reza R" first="R." last="De La Reza">R. De La Reza</name>
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<country>Brésil</country>
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<name sortKey="Dvorak, R" sort="Dvorak, R" uniqKey="Dvorak R" first="R." last="Dvorak">R. Dvorak</name>
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<name sortKey="Erikson, A" sort="Erikson, A" uniqKey="Erikson A" first="A." last="Erikson">A. Erikson</name>
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<inist:fA14 i1="09">
<s1>Institute of Planetary Research, DLR, Rutherfordstr. 2</s1>
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<author>
<name sortKey="Fridlund, M" sort="Fridlund, M" uniqKey="Fridlund M" first="M." last="Fridlund">M. Fridlund</name>
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<inist:fA14 i1="12">
<s1>Research and Scientific Support Department, European Space Agency, ESTEC</s1>
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<title xml:lang="en" level="a">Transiting exoplanets from the CoRoT space mission VI. CoRoT-Exo-3b : the first secure inhabitant of the brown-dwarf desert</title>
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<sZ>13 aut.</sZ>
<sZ>28 aut.</sZ>
<sZ>34 aut.</sZ>
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<author>
<name sortKey="Collier Cameron, A" sort="Collier Cameron, A" uniqKey="Collier Cameron A" first="A." last="Collier Cameron">A. Collier Cameron</name>
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<inist:fA14 i1="08">
<s1>School of Physics and Astronomy, University of St Andrews</s1>
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<sZ>14 aut.</sZ>
</inist:fA14>
<country>Royaume-Uni</country>
</affiliation>
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<author>
<name sortKey="Csizmadia, Sz" sort="Csizmadia, Sz" uniqKey="Csizmadia S" first="Sz." last="Csizmadia">Sz. Csizmadia</name>
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<inist:fA14 i1="09">
<s1>Institute of Planetary Research, DLR, Rutherfordstr. 2</s1>
<s2>12489 Berlin</s2>
<s3>DEU</s3>
<sZ>15 aut.</sZ>
<sZ>18 aut.</sZ>
<sZ>38 aut.</sZ>
</inist:fA14>
<country>Allemagne</country>
</affiliation>
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<author>
<name sortKey="De La Reza, R" sort="De La Reza, R" uniqKey="De La Reza R" first="R." last="De La Reza">R. De La Reza</name>
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<inist:fA14 i1="10">
<s1>Observatório Nacional</s1>
<s2>Rio de Janeiro, RJ</s2>
<s3>BRA</s3>
<sZ>16 aut.</sZ>
</inist:fA14>
<country>Brésil</country>
</affiliation>
</author>
<author>
<name sortKey="Dvorak, R" sort="Dvorak, R" uniqKey="Dvorak R" first="R." last="Dvorak">R. Dvorak</name>
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<inist:fA14 i1="11">
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<sZ>17 aut.</sZ>
</inist:fA14>
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<name sortKey="Erikson, A" sort="Erikson, A" uniqKey="Erikson A" first="A." last="Erikson">A. Erikson</name>
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<sZ>18 aut.</sZ>
<sZ>38 aut.</sZ>
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<author>
<name sortKey="Fridlund, M" sort="Fridlund, M" uniqKey="Fridlund M" first="M." last="Fridlund">M. Fridlund</name>
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<author>
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<sZ>22 aut.</sZ>
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<author>
<name sortKey="Gillon, M" sort="Gillon, M" uniqKey="Gillon M" first="M." last="Gillon">M. Gillon</name>
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<inist:fA14 i1="14">
<s1>Observatoire de Genève, Université de Genève, 51 Ch. des Maillettes</s1>
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<sZ>21 aut.</sZ>
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<name sortKey="Guenther, E" sort="Guenther, E" uniqKey="Guenther E" first="E." last="Guenther">E. Guenther</name>
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<s1>Thüringer Landesstemwarte Tautenburg, Sternwarte 5</s1>
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<sZ>22 aut.</sZ>
<sZ>24 aut.</sZ>
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<author>
<name sortKey="Guillot, T" sort="Guillot, T" uniqKey="Guillot T" first="T." last="Guillot">T. Guillot</name>
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<inist:fA14 i1="15">
<s1>Observatoire de la Côte d'Azur, Laboratoire Cassiopée, CNRS UMR 6202, BP 4229</s1>
<s2>06304 Nice</s2>
<s3>FRA</s3>
<sZ>23 aut.</sZ>
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<country>France</country>
</affiliation>
</author>
<author>
<name sortKey="Hatzes, A" sort="Hatzes, A" uniqKey="Hatzes A" first="A." last="Hatzes">A. Hatzes</name>
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<inist:fA14 i1="13">
<s1>Thüringer Landesstemwarte Tautenburg, Sternwarte 5</s1>
<s2>07778 Tautenburg</s2>
<s3>DEU</s3>
<sZ>20 aut.</sZ>
<sZ>22 aut.</sZ>
<sZ>24 aut.</sZ>
<sZ>41 aut.</sZ>
</inist:fA14>
<country>Allemagne</country>
</affiliation>
</author>
<author>
<name sortKey="Hebrard, G" sort="Hebrard, G" uniqKey="Hebrard G" first="G." last="Hebrard">G. Hebrard</name>
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<inist:fA14 i1="03">
<s1>Institut d'Astrophysique de Paris, UMR7095 CNRS, Université Pierre & Marie Curie, 98bis Bd Arago</s1>
<s2>75014 Paris</s2>
<s3>FRA</s3>
<sZ>4 aut.</sZ>
<sZ>25 aut.</sZ>
<sZ>30 aut.</sZ>
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<country>France</country>
</affiliation>
</author>
<author>
<name sortKey="Jorda, L" sort="Jorda, L" uniqKey="Jorda L" first="L." last="Jorda">L. Jorda</name>
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<inist:fA14 i1="01">
<s1>Laboratoire d'Astrophysique de Marseille (UMR 6110), Technopole de Marseille-Étoile</s1>
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<author>
<name sortKey="Lammer, H" sort="Lammer, H" uniqKey="Lammer H" first="H." last="Lammer">H. Lammer</name>
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<inist:fA14 i1="16">
<s1>Space Research Institute, Austrian Academy of Sciences, Schmiedlstrasse 6</s1>
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<name sortKey="Leger, A" sort="Leger, A" uniqKey="Leger A" first="A." last="Leger">A. Leger</name>
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<s1>IAS, Université Paris XI</s1>
<s2>91405 Orsay</s2>
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<sZ>28 aut.</sZ>
<sZ>34 aut.</sZ>
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<country>France</country>
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<author>
<name sortKey="Llebaria, A" sort="Llebaria, A" uniqKey="Llebaria A" first="A." last="Llebaria">A. Llebaria</name>
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<s1>Laboratoire d'Astrophysique de Marseille (UMR 6110), Technopole de Marseille-Étoile</s1>
<s2>13388 Marseille</s2>
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<country>France</country>
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<author>
<name sortKey="Loeillet, B" sort="Loeillet, B" uniqKey="Loeillet B" first="B." last="Loeillet">B. Loeillet</name>
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<inist:fA14 i1="01">
<s1>Laboratoire d'Astrophysique de Marseille (UMR 6110), Technopole de Marseille-Étoile</s1>
<s2>13388 Marseille</s2>
<s3>FRA</s3>
<sZ>1 aut.</sZ>
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<country>France</country>
</affiliation>
<affiliation wicri:level="1">
<inist:fA14 i1="03">
<s1>Institut d'Astrophysique de Paris, UMR7095 CNRS, Université Pierre & Marie Curie, 98bis Bd Arago</s1>
<s2>75014 Paris</s2>
<s3>FRA</s3>
<sZ>4 aut.</sZ>
<sZ>25 aut.</sZ>
<sZ>30 aut.</sZ>
</inist:fA14>
<country>France</country>
</affiliation>
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<author>
<name sortKey="Mayor, M" sort="Mayor, M" uniqKey="Mayor M" first="M." last="Mayor">M. Mayor</name>
<affiliation wicri:level="1">
<inist:fA14 i1="14">
<s1>Observatoire de Genève, Université de Genève, 51 Ch. des Maillettes</s1>
<s2>1290 Sauverny</s2>
<s3>CHE</s3>
<sZ>21 aut.</sZ>
<sZ>31 aut.</sZ>
<sZ>37 aut.</sZ>
</inist:fA14>
<country>Suisse</country>
</affiliation>
</author>
<author>
<name sortKey="Mazeh, T" sort="Mazeh, T" uniqKey="Mazeh T" first="T." last="Mazeh">T. Mazeh</name>
<affiliation wicri:level="1">
<inist:fA14 i1="17">
<s1>School of Physics and Astronomy, R. and B. Sackler Faculty of Exact Sciences, Tel Aviv University</s1>
<s2>Tel Aviv 69978</s2>
<s3>ISR</s3>
<sZ>32 aut.</sZ>
<sZ>40 aut.</sZ>
<sZ>42 aut.</sZ>
</inist:fA14>
<country>Israël</country>
</affiliation>
</author>
<author>
<name sortKey="Moutou, C" sort="Moutou, C" uniqKey="Moutou C" first="C." last="Moutou">C. Moutou</name>
<affiliation wicri:level="1">
<inist:fA14 i1="01">
<s1>Laboratoire d'Astrophysique de Marseille (UMR 6110), Technopole de Marseille-Étoile</s1>
<s2>13388 Marseille</s2>
<s3>FRA</s3>
<sZ>1 aut.</sZ>
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<sZ>10 aut.</sZ>
<sZ>11 aut.</sZ>
<sZ>26 aut.</sZ>
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<country>France</country>
</affiliation>
</author>
<author>
<name sortKey="Ollivier, M" sort="Ollivier, M" uniqKey="Ollivier M" first="M." last="Ollivier">M. Ollivier</name>
<affiliation wicri:level="1">
<inist:fA14 i1="07">
<s1>IAS, Université Paris XI</s1>
<s2>91405 Orsay</s2>
<s3>FRA</s3>
<sZ>13 aut.</sZ>
<sZ>28 aut.</sZ>
<sZ>34 aut.</sZ>
</inist:fA14>
<country>France</country>
</affiliation>
</author>
<author>
<name sortKey="P Tzold, M" sort="P Tzold, M" uniqKey="P Tzold M" first="M." last="P Tzold">M. P Tzold</name>
<affiliation wicri:level="1">
<inist:fA14 i1="18">
<s1>Rheinisches Institut für Umweltforschung, Universität zu Kôln, Abt. Planetenforschung, Aachener Str. 209</s1>
<s2>50931 Kôln</s2>
<s3>DEU</s3>
<sZ>35 aut.</sZ>
</inist:fA14>
<country>Allemagne</country>
</affiliation>
</author>
<author>
<name sortKey="Pont, F" sort="Pont, F" uniqKey="Pont F" first="F." last="Pont">F. Pont</name>
<affiliation wicri:level="1">
<inist:fA14 i1="05">
<s1>School of Physics, University of Exeter, Stocker Road</s1>
<s2>Exeter EX4 4QL</s2>
<s3>GBR</s3>
<sZ>8 aut.</sZ>
<sZ>36 aut.</sZ>
</inist:fA14>
<country>Royaume-Uni</country>
</affiliation>
</author>
<author>
<name sortKey="Queloz, D" sort="Queloz, D" uniqKey="Queloz D" first="D." last="Queloz">D. Queloz</name>
<affiliation wicri:level="1">
<inist:fA14 i1="14">
<s1>Observatoire de Genève, Université de Genève, 51 Ch. des Maillettes</s1>
<s2>1290 Sauverny</s2>
<s3>CHE</s3>
<sZ>21 aut.</sZ>
<sZ>31 aut.</sZ>
<sZ>37 aut.</sZ>
</inist:fA14>
<country>Suisse</country>
</affiliation>
</author>
<author>
<name sortKey="Rauer, H" sort="Rauer, H" uniqKey="Rauer H" first="H." last="Rauer">H. Rauer</name>
<affiliation wicri:level="1">
<inist:fA14 i1="09">
<s1>Institute of Planetary Research, DLR, Rutherfordstr. 2</s1>
<s2>12489 Berlin</s2>
<s3>DEU</s3>
<sZ>15 aut.</sZ>
<sZ>18 aut.</sZ>
<sZ>38 aut.</sZ>
</inist:fA14>
<country>Allemagne</country>
</affiliation>
<affiliation wicri:level="1">
<inist:fA14 i1="19">
<s1>Center for Astronomy and Astrophysics, TU Berlin, Hardenbergstr. 36</s1>
<s2>10623 Berlin</s2>
<s3>DEU</s3>
<sZ>38 aut.</sZ>
</inist:fA14>
<country>Allemagne</country>
</affiliation>
</author>
<author>
<name sortKey="Schneider, J" sort="Schneider, J" uniqKey="Schneider J" first="J." last="Schneider">J. Schneider</name>
<affiliation wicri:level="1">
<inist:fA14 i1="20">
<s1>LUTH, Observatoire de Paris-Meudon, 5 place J. Janssen</s1>
<s2>92195 Meudon</s2>
<s3>FRA</s3>
<sZ>39 aut.</sZ>
</inist:fA14>
<country>France</country>
</affiliation>
</author>
<author>
<name sortKey="Shporer, A" sort="Shporer, A" uniqKey="Shporer A" first="A." last="Shporer">A. Shporer</name>
<affiliation wicri:level="1">
<inist:fA14 i1="17">
<s1>School of Physics and Astronomy, R. and B. Sackler Faculty of Exact Sciences, Tel Aviv University</s1>
<s2>Tel Aviv 69978</s2>
<s3>ISR</s3>
<sZ>32 aut.</sZ>
<sZ>40 aut.</sZ>
<sZ>42 aut.</sZ>
</inist:fA14>
<country>Israël</country>
</affiliation>
</author>
<author>
<name sortKey="Wuchterl, G" sort="Wuchterl, G" uniqKey="Wuchterl G" first="G." last="Wuchterl">G. Wuchterl</name>
<affiliation wicri:level="1">
<inist:fA14 i1="13">
<s1>Thüringer Landesstemwarte Tautenburg, Sternwarte 5</s1>
<s2>07778 Tautenburg</s2>
<s3>DEU</s3>
<sZ>20 aut.</sZ>
<sZ>22 aut.</sZ>
<sZ>24 aut.</sZ>
<sZ>41 aut.</sZ>
</inist:fA14>
<country>Allemagne</country>
</affiliation>
</author>
<author>
<name sortKey="Zucker, S" sort="Zucker, S" uniqKey="Zucker S" first="S." last="Zucker">S. Zucker</name>
<affiliation wicri:level="1">
<inist:fA14 i1="17">
<s1>School of Physics and Astronomy, R. and B. Sackler Faculty of Exact Sciences, Tel Aviv University</s1>
<s2>Tel Aviv 69978</s2>
<s3>ISR</s3>
<sZ>32 aut.</sZ>
<sZ>40 aut.</sZ>
<sZ>42 aut.</sZ>
</inist:fA14>
<country>Israël</country>
</affiliation>
</author>
</analytic>
<series>
<title level="j" type="main">Astronomy and astrophysics : (Berlin. Print)</title>
<title level="j" type="abbreviated">Astron. astrophys. : (Berl., Print)</title>
<idno type="ISSN">0004-6361</idno>
<imprint>
<date when="2008">2008</date>
</imprint>
</series>
</biblStruct>
</sourceDesc>
<seriesStmt>
<title level="j" type="main">Astronomy and astrophysics : (Berlin. Print)</title>
<title level="j" type="abbreviated">Astron. astrophys. : (Berl., Print)</title>
<idno type="ISSN">0004-6361</idno>
</seriesStmt>
</fileDesc>
<profileDesc>
<textClass>
<keywords scheme="KwdEn" xml:lang="en">
<term>Brown dwarf stars</term>
<term>Extrasolar planets</term>
<term>Giant planet</term>
<term>Light curves</term>
<term>Low-mass stars</term>
<term>Massive stars</term>
<term>Orbits</term>
<term>Photometry</term>
<term>Planetary system</term>
<term>Radial velocity</term>
<term>Spectroscopical observation</term>
<term>Sun</term>
<term>Surface gravity</term>
</keywords>
<keywords scheme="Pascal" xml:lang="fr">
<term>Planète extrasolaire</term>
<term>Naine brune</term>
<term>Courbe lumière</term>
<term>Vitesse radiale</term>
<term>Photométrie</term>
<term>Observation spectroscopique</term>
<term>Orbite</term>
<term>Gravité surface</term>
<term>Planète géante</term>
<term>Etoile massive</term>
<term>Soleil</term>
<term>Système planétaire</term>
<term>Etoile faible masse</term>
</keywords>
</textClass>
</profileDesc>
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<front>
<div type="abstract" xml:lang="en">Context. The CoRoT space mission routinely provides high-precision photometric measurements of thousands of stars that have been continuously observed for months. Aims. The discovery and characterization of the first very massive transiting planetary companion with a short orbital period is reported. Methods. A series of 34 transits was detected in the CoRoT light curve of an F3V star, observed from May to October 2007 for 152 days. The radius was accurately determined and the mass derived for this new transiting, thanks to the combined analysis of the light curve and complementary ground-based observations: high-precision radial-velocity measurements, on-off photometry, and high signal-to-noise spectroscopic observations. Results. CoRoT-Exo-3b has a radius of 1.01 ± 0.07 R
<sub>Jup</sub>
and transits around its F3-type primary every 4.26 days in a synchronous orbit. Its mass of 21.66 ± 1.0M
<sub>Jup</sub>
, density of 26.4 ±5.6 g cm
<sup>-3</sup>
, and surface gravity of log g = 4.72 clearly distinguish it from the regular close-in planet population, making it the most intriguing transiting substellar object discovered so far. Conclusions. With the current data, the nature of CoRoT-Exo-3b is ambiguous, as it could either be a low-mass brown-dwarf or a member of a new class of "superplanets". Its discovery may help constrain the evolution of close-in planets and brown-dwarfs better. Finally, CoRoT-Exo-3b confirms the trend that massive transiting giant planets (M > 4 M
<sub>Jup</sub>
) are found preferentially around more massive stars than the Sun.</div>
</front>
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<s1>Transiting exoplanets from the CoRoT space mission VI. CoRoT-Exo-3b : the first secure inhabitant of the brown-dwarf desert</s1>
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<s1>DELEUIL (M.)</s1>
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</fA11>
<fA11 i1="15" i2="1">
<s1>CSIZMADIA (Sz.)</s1>
</fA11>
<fA11 i1="16" i2="1">
<s1>DE LA REZA (R.)</s1>
</fA11>
<fA11 i1="17" i2="1">
<s1>DVORAK (R.)</s1>
</fA11>
<fA11 i1="18" i2="1">
<s1>ERIKSON (A.)</s1>
</fA11>
<fA11 i1="19" i2="1">
<s1>FRIDLUND (M.)</s1>
</fA11>
<fA11 i1="20" i2="1">
<s1>GANDOLFI (D.)</s1>
</fA11>
<fA11 i1="21" i2="1">
<s1>GILLON (M.)</s1>
</fA11>
<fA11 i1="22" i2="1">
<s1>GUENTHER (E.)</s1>
</fA11>
<fA11 i1="23" i2="1">
<s1>GUILLOT (T.)</s1>
</fA11>
<fA11 i1="24" i2="1">
<s1>HATZES (A.)</s1>
</fA11>
<fA11 i1="25" i2="1">
<s1>HEBRARD (G.)</s1>
</fA11>
<fA11 i1="26" i2="1">
<s1>JORDA (L.)</s1>
</fA11>
<fA11 i1="27" i2="1">
<s1>LAMMER (H.)</s1>
</fA11>
<fA11 i1="28" i2="1">
<s1>LEGER (A.)</s1>
</fA11>
<fA11 i1="29" i2="1">
<s1>LLEBARIA (A.)</s1>
</fA11>
<fA11 i1="30" i2="1">
<s1>LOEILLET (B.)</s1>
</fA11>
<fA11 i1="31" i2="1">
<s1>MAYOR (M.)</s1>
</fA11>
<fA11 i1="32" i2="1">
<s1>MAZEH (T.)</s1>
</fA11>
<fA11 i1="33" i2="1">
<s1>MOUTOU (C.)</s1>
</fA11>
<fA11 i1="34" i2="1">
<s1>OLLIVIER (M.)</s1>
</fA11>
<fA11 i1="35" i2="1">
<s1>PÄTZOLD (M.)</s1>
</fA11>
<fA11 i1="36" i2="1">
<s1>PONT (F.)</s1>
</fA11>
<fA11 i1="37" i2="1">
<s1>QUELOZ (D.)</s1>
</fA11>
<fA11 i1="38" i2="1">
<s1>RAUER (H.)</s1>
</fA11>
<fA11 i1="39" i2="1">
<s1>SCHNEIDER (J.)</s1>
</fA11>
<fA11 i1="40" i2="1">
<s1>SHPORER (A.)</s1>
</fA11>
<fA11 i1="41" i2="1">
<s1>WUCHTERL (G.)</s1>
</fA11>
<fA11 i1="42" i2="1">
<s1>ZUCKER (S.)</s1>
</fA11>
<fA14 i1="01">
<s1>Laboratoire d'Astrophysique de Marseille (UMR 6110), Technopole de Marseille-Étoile</s1>
<s2>13388 Marseille</s2>
<s3>FRA</s3>
<sZ>1 aut.</sZ>
<sZ>3 aut.</sZ>
<sZ>10 aut.</sZ>
<sZ>11 aut.</sZ>
<sZ>26 aut.</sZ>
<sZ>29 aut.</sZ>
<sZ>30 aut.</sZ>
<sZ>33 aut.</sZ>
</fA14>
<fA14 i1="02">
<s1>Instituto de Astrofísica de Canarias, C. via Lactea S/N</s1>
<s2>38200 La Laguna</s2>
<s3>ESP</s3>
<sZ>2 aut.</sZ>
<sZ>9 aut.</sZ>
</fA14>
<fA14 i1="03">
<s1>Institut d'Astrophysique de Paris, UMR7095 CNRS, Université Pierre & Marie Curie, 98bis Bd Arago</s1>
<s2>75014 Paris</s2>
<s3>FRA</s3>
<sZ>4 aut.</sZ>
<sZ>25 aut.</sZ>
<sZ>30 aut.</sZ>
</fA14>
<fA14 i1="04">
<s1>LESIA, CNRS UMR 8109, Observatoire de Paris, 5 place J. Janssen</s1>
<s2>92195 Meudon</s2>
<s3>FRA</s3>
<sZ>5 aut.</sZ>
<sZ>6 aut.</sZ>
<sZ>7 aut.</sZ>
</fA14>
<fA14 i1="05">
<s1>School of Physics, University of Exeter, Stocker Road</s1>
<s2>Exeter EX4 4QL</s2>
<s3>GBR</s3>
<sZ>8 aut.</sZ>
<sZ>36 aut.</sZ>
</fA14>
<fA14 i1="06">
<s1>School of Physics A28, University of Sydney</s1>
<s3>AUS</s3>
<sZ>12 aut.</sZ>
</fA14>
<fA14 i1="07">
<s1>IAS, Université Paris XI</s1>
<s2>91405 Orsay</s2>
<s3>FRA</s3>
<sZ>13 aut.</sZ>
<sZ>28 aut.</sZ>
<sZ>34 aut.</sZ>
</fA14>
<fA14 i1="08">
<s1>School of Physics and Astronomy, University of St Andrews</s1>
<s3>GBR</s3>
<sZ>14 aut.</sZ>
</fA14>
<fA14 i1="09">
<s1>Institute of Planetary Research, DLR, Rutherfordstr. 2</s1>
<s2>12489 Berlin</s2>
<s3>DEU</s3>
<sZ>15 aut.</sZ>
<sZ>18 aut.</sZ>
<sZ>38 aut.</sZ>
</fA14>
<fA14 i1="10">
<s1>Observatório Nacional</s1>
<s2>Rio de Janeiro, RJ</s2>
<s3>BRA</s3>
<sZ>16 aut.</sZ>
</fA14>
<fA14 i1="11">
<s1>Institute for Astronomy, University of Vienna, Tûrkenschanzstrasse 17</s1>
<s2>1180 Vienna</s2>
<s3>AUT</s3>
<sZ>17 aut.</sZ>
</fA14>
<fA14 i1="12">
<s1>Research and Scientific Support Department, European Space Agency, ESTEC</s1>
<s2>2200 Noordwijk</s2>
<s3>NLD</s3>
<sZ>19 aut.</sZ>
</fA14>
<fA14 i1="13">
<s1>Thüringer Landesstemwarte Tautenburg, Sternwarte 5</s1>
<s2>07778 Tautenburg</s2>
<s3>DEU</s3>
<sZ>20 aut.</sZ>
<sZ>22 aut.</sZ>
<sZ>24 aut.</sZ>
<sZ>41 aut.</sZ>
</fA14>
<fA14 i1="14">
<s1>Observatoire de Genève, Université de Genève, 51 Ch. des Maillettes</s1>
<s2>1290 Sauverny</s2>
<s3>CHE</s3>
<sZ>21 aut.</sZ>
<sZ>31 aut.</sZ>
<sZ>37 aut.</sZ>
</fA14>
<fA14 i1="15">
<s1>Observatoire de la Côte d'Azur, Laboratoire Cassiopée, CNRS UMR 6202, BP 4229</s1>
<s2>06304 Nice</s2>
<s3>FRA</s3>
<sZ>23 aut.</sZ>
</fA14>
<fA14 i1="16">
<s1>Space Research Institute, Austrian Academy of Sciences, Schmiedlstrasse 6</s1>
<s2>8042 Graz</s2>
<s3>AUT</s3>
<sZ>27 aut.</sZ>
</fA14>
<fA14 i1="17">
<s1>School of Physics and Astronomy, R. and B. Sackler Faculty of Exact Sciences, Tel Aviv University</s1>
<s2>Tel Aviv 69978</s2>
<s3>ISR</s3>
<sZ>32 aut.</sZ>
<sZ>40 aut.</sZ>
<sZ>42 aut.</sZ>
</fA14>
<fA14 i1="18">
<s1>Rheinisches Institut für Umweltforschung, Universität zu Kôln, Abt. Planetenforschung, Aachener Str. 209</s1>
<s2>50931 Kôln</s2>
<s3>DEU</s3>
<sZ>35 aut.</sZ>
</fA14>
<fA14 i1="19">
<s1>Center for Astronomy and Astrophysics, TU Berlin, Hardenbergstr. 36</s1>
<s2>10623 Berlin</s2>
<s3>DEU</s3>
<sZ>38 aut.</sZ>
</fA14>
<fA14 i1="20">
<s1>LUTH, Observatoire de Paris-Meudon, 5 place J. Janssen</s1>
<s2>92195 Meudon</s2>
<s3>FRA</s3>
<sZ>39 aut.</sZ>
</fA14>
<fA20>
<s1>889-897</s1>
</fA20>
<fA21>
<s1>2008</s1>
</fA21>
<fA23 i1="01">
<s0>ENG</s0>
</fA23>
<fA43 i1="01">
<s1>INIST</s1>
<s2>14176</s2>
<s5>354000183994860280</s5>
</fA43>
<fA44>
<s0>0000</s0>
<s1>© 2009 INIST-CNRS. All rights reserved.</s1>
</fA44>
<fA45>
<s0>1/2 p.</s0>
</fA45>
<fA47 i1="01" i2="1">
<s0>09-0016503</s0>
</fA47>
<fA60>
<s1>P</s1>
</fA60>
<fA61>
<s0>A</s0>
</fA61>
<fA64 i1="01" i2="1">
<s0>Astronomy and astrophysics : (Berlin. Print)</s0>
</fA64>
<fA66 i1="01">
<s0>FRA</s0>
</fA66>
<fC01 i1="01" l="ENG">
<s0>Context. The CoRoT space mission routinely provides high-precision photometric measurements of thousands of stars that have been continuously observed for months. Aims. The discovery and characterization of the first very massive transiting planetary companion with a short orbital period is reported. Methods. A series of 34 transits was detected in the CoRoT light curve of an F3V star, observed from May to October 2007 for 152 days. The radius was accurately determined and the mass derived for this new transiting, thanks to the combined analysis of the light curve and complementary ground-based observations: high-precision radial-velocity measurements, on-off photometry, and high signal-to-noise spectroscopic observations. Results. CoRoT-Exo-3b has a radius of 1.01 ± 0.07 R
<sub>Jup</sub>
and transits around its F3-type primary every 4.26 days in a synchronous orbit. Its mass of 21.66 ± 1.0M
<sub>Jup</sub>
, density of 26.4 ±5.6 g cm
<sup>-3</sup>
, and surface gravity of log g = 4.72 clearly distinguish it from the regular close-in planet population, making it the most intriguing transiting substellar object discovered so far. Conclusions. With the current data, the nature of CoRoT-Exo-3b is ambiguous, as it could either be a low-mass brown-dwarf or a member of a new class of "superplanets". Its discovery may help constrain the evolution of close-in planets and brown-dwarfs better. Finally, CoRoT-Exo-3b confirms the trend that massive transiting giant planets (M > 4 M
<sub>Jup</sub>
) are found preferentially around more massive stars than the Sun.</s0>
</fC01>
<fC02 i1="01" i2="3">
<s0>001E03</s0>
</fC02>
<fC03 i1="01" i2="3" l="FRE">
<s0>Planète extrasolaire</s0>
<s5>26</s5>
</fC03>
<fC03 i1="01" i2="3" l="ENG">
<s0>Extrasolar planets</s0>
<s5>26</s5>
</fC03>
<fC03 i1="02" i2="3" l="FRE">
<s0>Naine brune</s0>
<s5>27</s5>
</fC03>
<fC03 i1="02" i2="3" l="ENG">
<s0>Brown dwarf stars</s0>
<s5>27</s5>
</fC03>
<fC03 i1="03" i2="3" l="FRE">
<s0>Courbe lumière</s0>
<s5>28</s5>
</fC03>
<fC03 i1="03" i2="3" l="ENG">
<s0>Light curves</s0>
<s5>28</s5>
</fC03>
<fC03 i1="04" i2="3" l="FRE">
<s0>Vitesse radiale</s0>
<s5>29</s5>
</fC03>
<fC03 i1="04" i2="3" l="ENG">
<s0>Radial velocity</s0>
<s5>29</s5>
</fC03>
<fC03 i1="05" i2="3" l="FRE">
<s0>Photométrie</s0>
<s5>30</s5>
</fC03>
<fC03 i1="05" i2="3" l="ENG">
<s0>Photometry</s0>
<s5>30</s5>
</fC03>
<fC03 i1="06" i2="X" l="FRE">
<s0>Observation spectroscopique</s0>
<s5>31</s5>
</fC03>
<fC03 i1="06" i2="X" l="ENG">
<s0>Spectroscopical observation</s0>
<s5>31</s5>
</fC03>
<fC03 i1="06" i2="X" l="SPA">
<s0>Observación espectroscópica</s0>
<s5>31</s5>
</fC03>
<fC03 i1="07" i2="3" l="FRE">
<s0>Orbite</s0>
<s5>32</s5>
</fC03>
<fC03 i1="07" i2="3" l="ENG">
<s0>Orbits</s0>
<s5>32</s5>
</fC03>
<fC03 i1="08" i2="3" l="FRE">
<s0>Gravité surface</s0>
<s5>33</s5>
</fC03>
<fC03 i1="08" i2="3" l="ENG">
<s0>Surface gravity</s0>
<s5>33</s5>
</fC03>
<fC03 i1="09" i2="X" l="FRE">
<s0>Planète géante</s0>
<s5>34</s5>
</fC03>
<fC03 i1="09" i2="X" l="ENG">
<s0>Giant planet</s0>
<s5>34</s5>
</fC03>
<fC03 i1="09" i2="X" l="SPA">
<s0>Planeta gigante</s0>
<s5>34</s5>
</fC03>
<fC03 i1="10" i2="3" l="FRE">
<s0>Etoile massive</s0>
<s5>35</s5>
</fC03>
<fC03 i1="10" i2="3" l="ENG">
<s0>Massive stars</s0>
<s5>35</s5>
</fC03>
<fC03 i1="11" i2="3" l="FRE">
<s0>Soleil</s0>
<s5>36</s5>
</fC03>
<fC03 i1="11" i2="3" l="ENG">
<s0>Sun</s0>
<s5>36</s5>
</fC03>
<fC03 i1="12" i2="X" l="FRE">
<s0>Système planétaire</s0>
<s5>37</s5>
</fC03>
<fC03 i1="12" i2="X" l="ENG">
<s0>Planetary system</s0>
<s5>37</s5>
</fC03>
<fC03 i1="12" i2="X" l="SPA">
<s0>Sistema planetario</s0>
<s5>37</s5>
</fC03>
<fC03 i1="13" i2="3" l="FRE">
<s0>Etoile faible masse</s0>
<s5>38</s5>
</fC03>
<fC03 i1="13" i2="3" l="ENG">
<s0>Low-mass stars</s0>
<s5>38</s5>
</fC03>
<fN21>
<s1>007</s1>
</fN21>
<fN44 i1="01">
<s1>OTO</s1>
</fN44>
<fN82>
<s1>OTO</s1>
</fN82>
</pA>
</standard>
</inist>
</record>

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