Issue |
A&A
Volume 585, January 2016
|
|
---|---|---|
Article Number | A126 | |
Number of page(s) | 7 | |
Section | Planets and planetary systems | |
DOI | https://doi.org/10.1051/0004-6361/201527276 | |
Published online | 08 January 2016 |
Three irradiated and bloated hot Jupiters:
WASP-76b, WASP-82b, and WASP-90b⋆
1
Department of PhysicsUniversity of Warwick,
Coventry
CV4 7AL,
UK
e-mail:
richard.west@warwick.ac.uk
2
Astrophysics Group, Keele University, Staffordshire, ST5 5BG, UK
3
Aix-Marseille Université, CNRS, LAM (Laboratoire d’Astrophysique
de Marseille) UMR 7326, 13388
Marseille,
France
4
Institut d’Astrophysique de Paris, UMR 7095 CNRS, Université
Pierre & Marie Curie, 75000
Paris,
France
5
Observatoire de Haute-Provence, CNRS/OAMP,
04870St. Michel l’Observatoire,
France
6
SUPA, School of Physics and Astronomy, University of St.
Andrews, North
Haugh, Fife,
KY16 9SS,
UK
7 Institut d’Astrophysique et de Géophysique, Université de
Liège, Allée du 6 Août 17, Bât. B5C, Liège 1, Belgium
8
Observatoire astronomique de l’Université de Genève,
51 Ch. des Maillettes,
1290
Sauverny,
Switzerland
9
Cavendish Laboratory, J J Thomson Avenue, Cambridge, CB3 0HE, UK
10
N. Copernicus Astronomical Centre, Polish Academy of
Sciences, Bartycka
18, 00-716
Warsaw,
Poland
11
Centre for Planetary Sciences, University of Toronto at
Scarborough, 1265 Military Trail,
Toronto, ON
M1C 1A4,
Canada
12
Department of Astronomy & Astrophysics, University of
Toronto, Toronto,
ON
M5S 3H4,
Canada
Received: 31 August 2015
Accepted: 8 October 2015
We report on three new transiting hot Jupiter planets, discovered from the WASP surveys, which we combine with radial velocities from OHP/SOPHIE and Euler/CORALIE and photometry from Euler and TRAPPIST. The planets WASP-76b, WASP-82b, and WASP-90b are all inflated, with radii of 1.7–1.8 RJup. All three orbit hot stars, of type F5–F7, with orbits of 1.8–3.9 d, and all three stars have evolved, post-main-sequence radii (1.7–2.2 R⊙). Thus the three planets fit a known trend of hot Jupiters that receive high levels of irradiation being highly inflated. We caution, though, about the presence of a selection effect, in that non-inflated planets around ~2 R⊙ post-MS stars can often produce transits too shallow to be detected by the ground-based surveys that have found the majority of transiting hot Jupiters.
Key words: planetary systems / stars: individual: WASP-76 / stars: individual: WASP-82 / stars: individual: WASP-90
Tables of the photometry and radial velocity are only available at the CDS via anonymous ftp to cdsarc.u-strasbg.fr (130.79.128.5) or via http://cdsarc.u-strasbg.fr/viz-bin/qcat?J/A+A/585/A126
© ESO, 2016
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