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Three Hot-Jupiters on the upper edge of the mass-radius distribution : WASP-177, WASP-181 and WASP-183

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dc.contributor.authorTurner, Oliver D.
dc.contributor.authorAnderson, D. R.
dc.contributor.authorBarkaoui, K.
dc.contributor.authorBouchy, F.
dc.contributor.authorBenkhaldoun, Z.
dc.contributor.authorBrown, D. J. A.
dc.contributor.authorBurdanov, A.
dc.contributor.authorCameron, A. Collier
dc.contributor.authorDucrot, E.
dc.contributor.authorGillon, M.
dc.contributor.authorHellier, C.
dc.contributor.authorJehin, E.
dc.contributor.authorLendl, M.
dc.contributor.authorMaxted, P. F. L.
dc.contributor.authorNielsen, L. D.
dc.contributor.authorPepe, F.
dc.contributor.authorPollacco, D.
dc.contributor.authorPozuelos, F. J.
dc.contributor.authorQueloz, D.
dc.contributor.authorSégransan, D.
dc.contributor.authorSmalley, B.
dc.contributor.authorTriaud, A. H. M. J.
dc.contributor.authorUdry, S.
dc.contributor.authorWest, R. G.
dc.date.accessioned2019-04-01T10:30:07Z
dc.date.available2019-04-01T10:30:07Z
dc.date.issued2019-06
dc.identifier.citationTurner , O D , Anderson , D R , Barkaoui , K , Bouchy , F , Benkhaldoun , Z , Brown , D J A , Burdanov , A , Cameron , A C , Ducrot , E , Gillon , M , Hellier , C , Jehin , E , Lendl , M , Maxted , P F L , Nielsen , L D , Pepe , F , Pollacco , D , Pozuelos , F J , Queloz , D , Ségransan , D , Smalley , B , Triaud , A H M J , Udry , S & West , R G 2019 , ' Three Hot-Jupiters on the upper edge of the mass-radius distribution : WASP-177, WASP-181 and WASP-183 ' , Monthly Notices of the Royal Astronomical Society , vol. 485 , no. 4 , pp. 5790–5799 . https://doi.org/10.1093/mnras/stz742en
dc.identifier.issn0035-8711
dc.identifier.otherPURE: 258412341
dc.identifier.otherPURE UUID: 3a712036-15e7-4fcd-bfd4-cd55eabb1a41
dc.identifier.otherArXiv: http://arxiv.org/abs/1903.06622v1
dc.identifier.otherORCID: /0000-0002-8863-7828/work/58531347
dc.identifier.otherWOS: 000474880400099
dc.identifier.otherScopus: 85072303894
dc.identifier.urihttp://hdl.handle.net/10023/17408
dc.descriptionThe research leading to these results has received funding from the European Research Council under the FP/2007-2013 ERC Grant Agreement 336480, from the ARC grant for Concerted Research Actions financed by the Wallonia-Brussels Federation, from the Balzan Foundation, and a grant from the Erasmus+ International Credit Mobility programme (K Barkaoui).en
dc.description.abstractWe present the discovery of 3 transiting planets from the WASP survey, two hot-Jupiters: WASP-177 b (∼0.5 MJup, ∼1.6 RJup) in a 3.07-d orbit of a V = 12.6 K2 star, WASP-183 b (∼0.5 MJup, ∼1.5 RJup) in a 4.11-d orbit of a V = 12.8 G9/K0 star; and one hot-Saturn planet WASP-181 b (∼0.3 MJup, ∼1.2 RJup) in a 4.52-d orbit of a V = 12.9 G2 star. Each planet is close to the upper bound of mass-radius space and has a scaled semi-major axis, a/R*, between 9.6 and 12.1. These lie in the transition between systems that tend to be in orbits that are well aligned with their host-star’s spin and those that show a higher dispersion.
dc.language.isoeng
dc.relation.ispartofMonthly Notices of the Royal Astronomical Societyen
dc.rights© 2019 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Society. This work has been made available online in accordance with the publisher's policies. This is the author created accepted version manuscript following peer review and as such may differ slightly from the final published version. The final published version of this work is available at https://doi.org/10.1093/mnras/stz742en
dc.subjectPlanets and satellites: detectionen
dc.subjectPlanets and satellites: individual: WASP-177ben
dc.subjectPlanets and satellites: individual: WASP-181ben
dc.subjectPlanets and satellites: individual: WASP-183ben
dc.subjectQB Astronomyen
dc.subjectQC Physicsen
dc.subjectDASen
dc.subject.lccQBen
dc.subject.lccQCen
dc.titleThree Hot-Jupiters on the upper edge of the mass-radius distribution : WASP-177, WASP-181 and WASP-183en
dc.typeJournal articleen
dc.description.versionPostprinten
dc.contributor.institutionUniversity of St Andrews. School of Physics and Astronomyen
dc.contributor.institutionUniversity of St Andrews. St Andrews Centre for Exoplanet Scienceen
dc.identifier.doihttps://doi.org/10.1093/mnras/stz742
dc.description.statusPeer revieweden


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