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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.author | Turner, Oliver D. | |
dc.contributor.author | Anderson, D. R. | |
dc.contributor.author | Barkaoui, K. | |
dc.contributor.author | Bouchy, F. | |
dc.contributor.author | Benkhaldoun, Z. | |
dc.contributor.author | Brown, D. J. A. | |
dc.contributor.author | Burdanov, A. | |
dc.contributor.author | Cameron, A. Collier | |
dc.contributor.author | Ducrot, E. | |
dc.contributor.author | Gillon, M. | |
dc.contributor.author | Hellier, C. | |
dc.contributor.author | Jehin, E. | |
dc.contributor.author | Lendl, M. | |
dc.contributor.author | Maxted, P. F. L. | |
dc.contributor.author | Nielsen, L. D. | |
dc.contributor.author | Pepe, F. | |
dc.contributor.author | Pollacco, D. | |
dc.contributor.author | Pozuelos, F. J. | |
dc.contributor.author | Queloz, D. | |
dc.contributor.author | Ségransan, D. | |
dc.contributor.author | Smalley, B. | |
dc.contributor.author | Triaud, A. H. M. J. | |
dc.contributor.author | Udry, S. | |
dc.contributor.author | West, R. G. | |
dc.date.accessioned | 2019-04-01T10:30:07Z | |
dc.date.available | 2019-04-01T10:30:07Z | |
dc.date.issued | 2019-06 | |
dc.identifier | 258412341 | |
dc.identifier | 3a712036-15e7-4fcd-bfd4-cd55eabb1a41 | |
dc.identifier | 000474880400099 | |
dc.identifier | 85072303894 | |
dc.identifier.citation | Turner , 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/stz742 | en |
dc.identifier.issn | 0035-8711 | |
dc.identifier.other | ArXiv: http://arxiv.org/abs/1903.06622v1 | |
dc.identifier.other | ORCID: /0000-0002-8863-7828/work/58531347 | |
dc.identifier.uri | https://hdl.handle.net/10023/17408 | |
dc.description | The 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.abstract | We 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.format.extent | 1002514 | |
dc.language.iso | eng | |
dc.relation.ispartof | Monthly Notices of the Royal Astronomical Society | en |
dc.subject | Planets and satellites: detection | en |
dc.subject | Planets and satellites: individual: WASP-177b | en |
dc.subject | Planets and satellites: individual: WASP-181b | en |
dc.subject | Planets and satellites: individual: WASP-183b | en |
dc.subject | QB Astronomy | en |
dc.subject | QC Physics | en |
dc.subject | DAS | en |
dc.subject.lcc | QB | en |
dc.subject.lcc | QC | en |
dc.title | Three Hot-Jupiters on the upper edge of the mass-radius distribution : WASP-177, WASP-181 and WASP-183 | en |
dc.type | Journal article | en |
dc.contributor.institution | University of St Andrews. School of Physics and Astronomy | en |
dc.contributor.institution | University of St Andrews. St Andrews Centre for Exoplanet Science | en |
dc.identifier.doi | 10.1093/mnras/stz742 | |
dc.description.status | Peer reviewed | en |
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