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WASP-135b : a highly irradiated, inflated hot Jupiter orbiting a G5V star

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dc.contributor.authorSpake, Jessica J.
dc.contributor.authorBrown, David John Alexander
dc.contributor.authorDoyle, Amanda P.
dc.contributor.authorHébrard, Guillaume
dc.contributor.authorMcCormac, James
dc.contributor.authorArmstrong, David J.
dc.contributor.authorPollacco, Don
dc.contributor.authorChew, Yilen Gómez Maqueo
dc.contributor.authorAnderson, David R.
dc.contributor.authorBarros, Susana C. C.
dc.contributor.authorBouchy, François
dc.contributor.authorBoumis, Panayotis
dc.contributor.authorBruno, Giovanni
dc.contributor.authorCameron, Andrew Collier
dc.contributor.authorCourcol, Bastien
dc.contributor.authorDavies, Guy R.
dc.contributor.authorFaedi, Francesca
dc.contributor.authorHellier, Coel
dc.contributor.authorKirk, James
dc.contributor.authorLam, Kristine W. F.
dc.contributor.authorLiakos, Alexios
dc.contributor.authorLouden, Tom
dc.contributor.authorMaxted, Pierre F. L.
dc.contributor.authorOsborn, Hugh P.
dc.contributor.authorPalle, Enric
dc.contributor.authorArranz, Jorge Prieto
dc.contributor.authorUdry, Stéphane
dc.contributor.authorWalker, Simon R.
dc.contributor.authorWest, Richard G.
dc.contributor.authorWheatley, Peter J.
dc.date.accessioned2016-02-05T14:40:10Z
dc.date.available2016-02-05T14:40:10Z
dc.date.issued2016-01-14
dc.identifier240467198
dc.identifier45608cac-3e71-4b33-831a-dbaea1c84517
dc.identifier84973531860
dc.identifier000387106800002
dc.identifier.citationSpake , J J , Brown , D J A , Doyle , A P , Hébrard , G , McCormac , J , Armstrong , D J , Pollacco , D , Chew , Y G M , Anderson , D R , Barros , S C C , Bouchy , F , Boumis , P , Bruno , G , Cameron , A C , Courcol , B , Davies , G R , Faedi , F , Hellier , C , Kirk , J , Lam , K W F , Liakos , A , Louden , T , Maxted , P F L , Osborn , H P , Palle , E , Arranz , J P , Udry , S , Walker , S R , West , R G & Wheatley , P J 2016 , ' WASP-135b : a highly irradiated, inflated hot Jupiter orbiting a G5V star ' , Publications of the Astronomical Society of the Pacific , vol. 128 , no. 960 . https://doi.org/10.1088/1538-3873/128/960/024401en
dc.identifier.issn0004-6280
dc.identifier.otherArXiv: http://arxiv.org/abs/1511.05954v1
dc.identifier.otherORCID: /0000-0002-8863-7828/work/58531320
dc.identifier.urihttps://hdl.handle.net/10023/8151
dc.description.abstractWe report the discovery of a new transiting planet from the WASP survey. WASP-135b is a hot Jupiter with a radius of 1.30 pm 0.09 Rjup, a mass of 1.90 pm 0.08 Mjup and an orbital period of 1.401 days. Its host is a Sun-like star, with a G5 spectral type and a mass and radius of 0.98 pm 0.06 Msun and 0.96 pm 0.05 Rsun respectively. The proximity of the planet to its host means that WASP-135b receives high levels of insolation, which may be the cause of its inflated radius. Additionally, we find weak evidence of a transfer of angular momentum from the planet to its star.
dc.format.extent512078
dc.language.isoeng
dc.relation.ispartofPublications of the Astronomical Society of the Pacificen
dc.subjectExtrasolar planetsen
dc.subjectStars: individual: WASP-135en
dc.subjectTechniques: radial velocity, photometryen
dc.subjectQB Astronomyen
dc.subjectQC Physicsen
dc.subject3rd-DASen
dc.subject.lccQBen
dc.subject.lccQCen
dc.titleWASP-135b : a highly irradiated, inflated hot Jupiter orbiting a G5V staren
dc.typeJournal articleen
dc.contributor.sponsorScience & Technology Facilities Councilen
dc.contributor.sponsorScience & Technology Facilities Councilen
dc.contributor.institutionUniversity of St Andrews. School of Physics and Astronomyen
dc.identifier.doi10.1088/1538-3873/128/960/024401
dc.description.statusPeer revieweden
dc.identifier.grantnumberST/M001296/1en
dc.identifier.grantnumberST/J001651/1en


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