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WASP-104b and WASP-106b : two transiting hot Jupiters in 1.75-day and 9.3-day orbits
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dc.contributor.author | Smith, A.M.S. | |
dc.contributor.author | Anderson, D.R. | |
dc.contributor.author | Armstrong, D.J. | |
dc.contributor.author | Barros, S.C.C. | |
dc.contributor.author | Bonomo, A.S. | |
dc.contributor.author | Bouchy, F. | |
dc.contributor.author | Brown, D.J.A. | |
dc.contributor.author | Collier Cameron, A. | |
dc.contributor.author | Delrez, L. | |
dc.contributor.author | Faedi, F. | |
dc.contributor.author | Gillon, M. | |
dc.contributor.author | Gómez Maqueo Chew, Y. | |
dc.contributor.author | Hébrard, G. | |
dc.contributor.author | Jehin, E. | |
dc.contributor.author | Lendl, M. | |
dc.contributor.author | Louden, T.M. | |
dc.contributor.author | Maxted, P.F.L. | |
dc.contributor.author | Montagnier, G. | |
dc.contributor.author | Neveu-Vanmalle, M. | |
dc.contributor.author | Osborn, H.P. | |
dc.contributor.author | Pepe, F. | |
dc.contributor.author | Pollacco, D. | |
dc.contributor.author | Queloz, D. | |
dc.contributor.author | Rostron, J.W. | |
dc.contributor.author | Segransan, D. | |
dc.contributor.author | Smalley, B. | |
dc.contributor.author | Triaud, A.H.M.J. | |
dc.contributor.author | Turner, O.D. | |
dc.contributor.author | Udry, S. | |
dc.contributor.author | Walker, S.R. | |
dc.contributor.author | West, R.G. | |
dc.contributor.author | Wheatley, P.J. | |
dc.date.accessioned | 2014-12-16T17:01:02Z | |
dc.date.available | 2014-12-16T17:01:02Z | |
dc.date.issued | 2014-10 | |
dc.identifier.citation | Smith , A M S , Anderson , D R , Armstrong , D J , Barros , S C C , Bonomo , A S , Bouchy , F , Brown , D J A , Collier Cameron , A , Delrez , L , Faedi , F , Gillon , M , Gómez Maqueo Chew , Y , Hébrard , G , Jehin , E , Lendl , M , Louden , T M , Maxted , P F L , Montagnier , G , Neveu-Vanmalle , M , Osborn , H P , Pepe , F , Pollacco , D , Queloz , D , Rostron , J W , Segransan , D , Smalley , B , Triaud , A H M J , Turner , O D , Udry , S , Walker , S R , West , R G & Wheatley , P J 2014 , ' WASP-104b and WASP-106b : two transiting hot Jupiters in 1.75-day and 9.3-day orbits ' , Astronomy & Astrophysics , vol. 570 , A64 . https://doi.org/10.1051/0004-6361/201424752 | en |
dc.identifier.issn | 0004-6361 | |
dc.identifier.other | PURE: 158989558 | |
dc.identifier.other | PURE UUID: 266e7e69-5e52-41ff-9702-264b1afed3c3 | |
dc.identifier.other | Scopus: 84907946061 | |
dc.identifier.other | ORCID: /0000-0002-8863-7828/work/58531315 | |
dc.identifier.other | WOS: 000344158500139 | |
dc.identifier.uri | https://hdl.handle.net/10023/5928 | |
dc.description | Funding for WASP comes from consortium universities and from the UK’s Science and Technology Facilities Council (STFC). | en |
dc.description.abstract | We have used the WASP survey to discover two exoplanetary systems, each consisting of a Jupiter-sized planet transiting an 11th-magnitude (V) main-sequence star. WASP-104b orbits its star in 1.75 d, whereas WASP-106b has the fourth-longest orbital period of any planet discovered by means of transits observed from the ground, orbiting every 9.29 d. Each planet is more massive than Jupiter (WASP-104b has a mass of 1.27 ± 0.05MJup, while WASP-106b has a mass of 1.93 ± 0.08MJup). Both planets are just slightly larger than Jupiter, with radii of 1.14 ± 0.04 and 1.09 ± 0.04RJup for WASP-104 and WASP-106, respectively. No significant orbital eccentricity is detected in either system, and while this is not surprising in the case of the short-period WASP-104b, it is interesting in the case of WASP-106b, because many otherwise similar planets are known to have eccentric orbits. | |
dc.format.extent | 8 | |
dc.language.iso | eng | |
dc.relation.ispartof | Astronomy & Astrophysics | en |
dc.rights | Reproduced with permission from Astronomy & Astrophysics, © ESO | en |
dc.subject | Planets and satellites: detection | en |
dc.subject | Planets and satellites: fundamental parameters | en |
dc.subject | Stars: individual: WASP-104b | en |
dc.subject | Stars: individual: WASP-106b | en |
dc.subject | Planetary systems | en |
dc.subject | QB Astronomy | en |
dc.subject | QC Physics | en |
dc.subject.lcc | QB | en |
dc.subject.lcc | QC | en |
dc.title | WASP-104b and WASP-106b : two transiting hot Jupiters in 1.75-day and 9.3-day orbits | en |
dc.type | Journal article | en |
dc.contributor.sponsor | Science & Technology Facilities Council | en |
dc.contributor.sponsor | Science & Technology Facilities Council | en |
dc.description.version | Publisher PDF | en |
dc.contributor.institution | University of St Andrews. School of Physics and Astronomy | en |
dc.identifier.doi | https://doi.org/10.1051/0004-6361/201424752 | |
dc.description.status | Peer reviewed | en |
dc.identifier.grantnumber | ST/J001651/1 | en |
dc.identifier.grantnumber | PP/F000065/1 | en |
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