2008A&A...491..889D


C.D.S. - SIMBAD4 rel 1.7 - 2019.10.21CEST05:52:44

2008A&A...491..889D - Astronomy and Astrophysics, volume 491, 889-897 (2008/12-1)

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

DELEUIL M., DEEG H.J., ALONSO R., BOUCHY F., ROUAN D., AUVERGNE M., BAGLIN A., AIGRAIN S., ALMENARA J.M., BARBIERI M., BARGE P., BRUNTT H., BORDE P., COLLIER CAMERON A., CSIZMADIA Sz., DE LA REZA R., DVORAK R., ERIKSON A., FRIDLUND M., GANDOLFI D., GILLON M., GUENTHER E., GUILLOT T., HATZES A., HEBRARD G., JORDA L., LAMMER H., LEGER A., LLEBARIA A., LOEILLET B., MAYOR M., MAZEH T., MOUTOU C., OLLIVIER M., PAETZOLD M., PONT F., QUELOZ D., RAUER H., SCHNEIDER J., SHPORER A., WUCHTERL G. and ZUCKER S.

Abstract (from CDS):

The CoRoT space mission routinely provides high-precision photometric measurements of thousands of stars that have been continuously observed for months. The discovery and characterization of the first very massive transiting planetary companion with a short orbital period is reported. 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. CoRoT-Exo-3b has a radius of 1.01±0.07RJup 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±5.6g/cm3, and surface gravity of logg=4.72 clearly distinguish it from the regular close-in planet population, making it the most intriguing transiting substellar object discovered so far. 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≥4MJup) are found preferentially around more massive stars than the Sun.

Abstract Copyright:

Journal keyword(s): stars: planetary systems - stars: low-mass, brown-dwarfs - Sun: fundamental parameters

VizieR on-line data: <Available at CDS (J/A+A/491/889): table.dat table.fits>

Nomenclature: CoRoT-N (No. 3), CoRoT-Na (No. 3b).

Simbad objects: 13

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Number of rows : 13

N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2019
#notes
1 XO-3b Pl 04 21 52.7044170433 +57 49 01.892074012           ~ 167 1
2 XO-3 * 04 21 52.7044170433 +57 49 01.892074012   10.27 9.85     F5V 128 2
3 HD 41004B * 05 59 49.649 -48 14 22.88   13.85 12.33     M 48 1
4 CoRoT-4b Pl 06 48 46.7133639143 -00 40 21.969520601           ~ 56 1
5 * tau Boo ** 13 47 15.74340 +17 27 24.8552 5.02 4.98 4.49 4.09 3.85 F7IV-V 862 1
6 BD+22 2716b Pl 14 33 06.3573673505 +21 53 40.982782397           ~ 114 1
7 BD+22 2716 * 14 33 06.3573673505 +21 53 40.982782397   10.194 9.745     F5V 78 1
8 * 37 Lib PM* 15 34 10.7020905 -10 03 52.306353 6.48 5.63 4.62 3.85 3.33 K1III-IV 155 0
9 HD 147506b Pl 16 20 36.3579144486 +41 02 53.109043943           ~ 205 1
10 HD 147506 * 16 20 36.3579144486 +41 02 53.109043943   9.15 8.69     F8V 135 2
11 HD 162020 * 17 50 38.3545681675 -40 19 06.080050505   10.11 9.12     K3V 124 1
12 CoRoT-3 EB* 19 28 13.2642482783 +00 07 18.614302248   14.199 13.292 13.099 12.54 F3V 65 1
13 CoRoT-3b Pl 19 28 13.2642482783 +00 07 18.614302248           ~ 111 1

    Equat.    Gal    SGal    Ecl

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2019.10.21-05:52:44

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