Three irradiated and bloated hot Jupiters: WASP-76b, WASP-82b, and WASP-90b

R. G. West; C. Hellier; J.-M. Almenara; D. R. Anderson; S. C. C. Barros; F. Bouchy; D. J. A. Brown; A. Collier Cameron; M. Deleuil; L. Delrez; A. P. Doyle; F. Faedi; A. Fumel; M. Gillon; Y. Gómez Maqueo Chew; G. Hébrard; E. Jehin; M. Lendl; P. F. L. Maxted; F. Pepe; D. Pollacco; D. Queloz; D. Ségransan; B. Smalley; A. M. S. Smith; J. Southworth; A. H. M. J. Triaud; S. Udry

doi:10.1051/0004-6361/201527276

Three irradiated and bloated hot Jupiters: WASP-76b, WASP-82b, and WASP-90b

R. G. West
, C. Hellier
, J.-M. Almenara
, D. R. Anderson
, S. C. C. Barros
, F. Bouchy
, D. J. A. Brown
, A. Collier Cameron
, M. Deleuil
, L. Delrez
, A. P. Doyle
, F. Faedi
, A. Fumel
, M. Gillon
, Y. Gómez Maqueo Chew
, G. Hébrard
, E. Jehin
, M. Lendl
, P. F. L. Maxted
, F. Pepe

D. Pollacco, D. Queloz, D. Ségransan, B. Smalley, A. M. S. Smith, J. Southworth, A. H. M. J. Triaud, S. Udry

School of Physics and Astronomy

Research output: Contribution to journal › Article › peer-review

Abstract

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.

Original language	English
Article number	A126
Number of pages	7
Journal	Astronomy & Astrophysics
Volume	585
DOIs	https://doi.org/10.1051/0004-6361/201527276
Publication status	Published - 8 Jan 2016

Keywords

Planetary systems
Stars: individual: WASP-76
Stars: individual: WASP-82
Stars: individual: WASP-90

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West, R. G., Hellier, C., Almenara, J.-M., Anderson, D. R., Barros, S. C. C., Bouchy, F., Brown, D. J. A., Collier Cameron, A., Deleuil, M., Delrez, L., Doyle, A. P., Faedi, F., Fumel, A., Gillon, M., Gómez Maqueo Chew, Y., Hébrard, G., Jehin, E., Lendl, M., Maxted, P. F. L., ... Udry, S. (2016). Three irradiated and bloated hot Jupiters: WASP-76b, WASP-82b, and WASP-90b. Astronomy & Astrophysics, 585, Article A126. https://doi.org/10.1051/0004-6361/201527276

@article{9e970b3946c64e39bfbfd5d332dbbb98,

title = "Three irradiated and bloated hot Jupiters: WASP-76b, WASP-82b, and WASP-90b",

abstract = "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 \textasciitilde{}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.",

keywords = "Planetary systems, Stars: individual: WASP-76 , Stars: individual: WASP-82, Stars: individual: WASP-90",

author = "West, \{R. G.\} and C. Hellier and J.-M. Almenara and Anderson, \{D. R.\} and Barros, \{S. C. C.\} and F. Bouchy and Brown, \{D. J. A.\} and \{Collier Cameron\}, A. and M. Deleuil and L. Delrez and Doyle, \{A. P.\} and F. Faedi and A. Fumel and M. Gillon and \{G{\'o}mez Maqueo Chew\}, Y. and G. H{\'e}brard and E. Jehin and M. Lendl and Maxted, \{P. F. L.\} and F. Pepe and D. Pollacco and D. Queloz and D. S{\'e}gransan and B. Smalley and Smith, \{A. M. S.\} and J. Southworth and Triaud, \{A. H. M. J.\} and S. Udry",

year = "2016",

month = jan,

day = "8",

doi = "10.1051/0004-6361/201527276",

language = "English",

volume = "585",

journal = "Astronomy \& Astrophysics",

issn = "0004-6361",

publisher = "EDP Sciences",

}

West, RG, Hellier, C, Almenara, J-M, Anderson, DR, Barros, SCC, Bouchy, F, Brown, DJA, Collier Cameron, A, Deleuil, M, Delrez, L, Doyle, AP, Faedi, F, Fumel, A, Gillon, M, Gómez Maqueo Chew, Y, Hébrard, G, Jehin, E, Lendl, M, Maxted, PFL, Pepe, F, Pollacco, D, Queloz, D, Ségransan, D, Smalley, B, Smith, AMS, Southworth, J, Triaud, AHMJ & Udry, S 2016, 'Three irradiated and bloated hot Jupiters: WASP-76b, WASP-82b, and WASP-90b', Astronomy & Astrophysics, vol. 585, A126. https://doi.org/10.1051/0004-6361/201527276

TY - JOUR

T1 - Three irradiated and bloated hot Jupiters: WASP-76b, WASP-82b, and WASP-90b

AU - West, R. G.

AU - Hellier, C.

AU - Almenara, J.-M.

AU - Anderson, D. R.

AU - Barros, S. C. C.

AU - Bouchy, F.

AU - Brown, D. J. A.

AU - Collier Cameron, A.

AU - Deleuil, M.

AU - Delrez, L.

AU - Doyle, A. P.

AU - Faedi, F.

AU - Fumel, A.

AU - Gillon, M.

AU - Gómez Maqueo Chew, Y.

AU - Hébrard, G.

AU - Jehin, E.

AU - Lendl, M.

AU - Maxted, P. F. L.

AU - Pepe, F.

AU - Pollacco, D.

AU - Queloz, D.

AU - Ségransan, D.

AU - Smalley, B.

AU - Smith, A. M. S.

AU - Southworth, J.

AU - Triaud, A. H. M. J.

AU - Udry, S.

PY - 2016/1/8

Y1 - 2016/1/8

N2 - 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.

AB - 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.

KW - Planetary systems

KW - Stars: individual: WASP-76

KW - Stars: individual: WASP-82

KW - Stars: individual: WASP-90

UR - http://adsabs.harvard.edu/abs/2013arXiv1310.5607W

U2 - 10.1051/0004-6361/201527276

DO - 10.1051/0004-6361/201527276

M3 - Article

SN - 0004-6361

VL - 585

JO - Astronomy & Astrophysics

JF - Astronomy & Astrophysics

M1 - A126

ER -

Three irradiated and bloated hot Jupiters: WASP-76b, WASP-82b, and WASP-90b

Abstract

Keywords

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Astronomy at St Andrews 2015-2018: Astronomy at St Andrews 2015-2018

Astrophysics at St Andrews:2012 - 2014: Astrophysics at St Andrews: 2012 - 2014

Wide Area Search for Planets: Project support for the Wide Area Search for Planets

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Three irradiated and bloated hot Jupiters: WASP-76b, WASP-82b, and WASP-90b

Abstract

Keywords

Access to Document

Handle.net

Other files and links

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Projects

Astronomy at St Andrews 2015-2018: Astronomy at St Andrews 2015-2018

Astrophysics at St Andrews:2012 - 2014: Astrophysics at St Andrews: 2012 - 2014

Wide Area Search for Planets: Project support for the Wide Area Search for Planets

Cite this