2010A&A...524A..55G


C.D.S. - SIMBAD4 rel 1.7 - 2019.11.18CET00:39:13

2010A&A...524A..55G - Astronomy and Astrophysics, volume 524, A55-55 (2010/12-1)

Transiting exoplanets from the CoRoT space mission. XIV. CoRoT-11b: a transiting massive ``hot-Jupiter'' in a prograde orbit around a rapidly rotating F-type star.

GANDOLFI D., HEBRARD G., ALONSO R., DELEUIL M., GUENTHER E.W., FRIDLUND M., ENDL M., EIGMUELLER P., CSIZMADIA Sz., HAVEL M., AIGRAIN S., AUVERGNE M., BAGLIN A., BARGE P., BONOMO A.S., BORDE P., BOUCHY F., BRUNTT H., CABRERA J., CARPANO S., CARONE L., COCHRAN W.D., DEEG H.J., DVORAK R., EISLOEFFEL J., ERIKSON A., FERRAZ-MELLO S., GAZZANO J.-C., GIBSON N.B., GILLON M., GONDOIN P., GUILLOT T., HARTMANN M., HATZES A., JORDA L., KABATH P., LEGER A., LLEBARIA A., LAMMER H., MacQUEEN P.J., MAYOR M., MAZEH T., MOUTOU C., OLLIVIER M., PAETZOLD M., PEPE F., QUELOZ D., RAUER H., ROUAN D., SAMUEL B., SCHNEIDER J., STECKLUM B., TINGLEY B., UDRY S. and WUCHTERL G.

Abstract (from CDS):

The CoRoT exoplanet science team announces the discovery of CoRoT-11b, a fairly massive hot-Jupiter transiting a V=12.9mag F6 dwarf star (M*=1.27±0.05M, R*=1.37±0.03R, Teff=6440±120K), with an orbital period of P=2.994329±0.000011-days and semi-major axis a=0.0436±0.005AU. The detection of part of the radial velocity anomaly caused by the Rossiter-McLaughlin effect shows that the transit-like events detected by CoRoT are caused by a planet-sized transiting object in a prograde orbit. The relatively high projected rotational velocity of the star (vsini*=40±5km/s) places CoRoT-11 among the most rapidly rotating planet host stars discovered so far. With a planetary mass of Mp=2.33±0.34MJup and radius Rp=1.43±0.03RJup, the resulting mean density of CoRoT-11b (ρp=0.99±0.15g/cm3) can be explained with a model for an inflated hydrogen-planet with a solar composition and a high level of energy dissipation in its interior.

Abstract Copyright:

Journal keyword(s): planetary systems - techniques: photometric - techniques: radial velocities - techniques: spectroscopic

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 - 2020
#notes
1 NGC 752 OpC 01 57 41 +37 47.1           ~ 526 0
2 HD 15082b Pl 02 26 51.0582746497 +37 33 01.737746137           ~ 156 1
3 * 30 Ari Bb Pl 02 36 57.7448892346 +24 38 53.002647458           ~ 15 1
4 Cl Melotte 22 OpC 03 47 00 +24 07.0           ~ 2912 0
5 Cl Melotte 25 OpC 04 26 54.00 +15 52 00.0           ~ 2586 0
6 NAME OGLE2-TR-L9b Pl 11 07 55.181 -61 08 46.58           ~ 22 1
7 * 37 Lib PM* 15 34 10.7020905 -10 03 52.306353 6.48 5.63 4.62 3.85 3.33 K1III-IV 156 0
8 NAME Ophiuchus Molecular Cloud SFR 16 28 06 -24 32.5           ~ 2938 0
9 NAME Gal Center reg 17 45 40.04 -29 00 28.1           ~ 11047 0
10 NAME Serpens Cloud SFR 18 29 49 +01 14.8           ~ 885 2
11 CoRoT-11 EB* 18 42 44.9499508376 +05 56 15.652163640   13.73 12.939     F6V 41 1
12 CoRoT-11b Pl 18 42 44.9499508376 +05 56 15.652163640           ~ 35 1
13 CoRoT-2b Pl 19 27 06.4944821296 +01 23 01.357597206     12.57     ~ 170 1

    Equat.    Gal    SGal    Ecl

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2019.11.18-00:39:13

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