Show simple item record

Files in this item


Item metadata

dc.contributor.authorSmith, A.M.S.
dc.contributor.authorAnderson, D.R.
dc.contributor.authorArmstrong, D.J.
dc.contributor.authorBarros, S.C.C.
dc.contributor.authorBonomo, A.S.
dc.contributor.authorBouchy, F.
dc.contributor.authorBrown, D.J.A.
dc.contributor.authorCollier Cameron, A.
dc.contributor.authorDelrez, L.
dc.contributor.authorFaedi, F.
dc.contributor.authorGillon, M.
dc.contributor.authorGómez Maqueo Chew, Y.
dc.contributor.authorHébrard, G.
dc.contributor.authorJehin, E.
dc.contributor.authorLendl, M.
dc.contributor.authorLouden, T.M.
dc.contributor.authorMaxted, P.F.L.
dc.contributor.authorMontagnier, G.
dc.contributor.authorNeveu-Vanmalle, M.
dc.contributor.authorOsborn, H.P.
dc.contributor.authorPepe, F.
dc.contributor.authorPollacco, D.
dc.contributor.authorQueloz, D.
dc.contributor.authorRostron, J.W.
dc.contributor.authorSegransan, D.
dc.contributor.authorSmalley, B.
dc.contributor.authorTriaud, A.H.M.J.
dc.contributor.authorTurner, O.D.
dc.contributor.authorUdry, S.
dc.contributor.authorWalker, S.R.
dc.contributor.authorWest, R.G.
dc.contributor.authorWheatley, P.J.
dc.identifier.citationSmith , 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 .
dc.identifier.otherPURE: 158989558
dc.identifier.otherPURE UUID: 266e7e69-5e52-41ff-9702-264b1afed3c3
dc.identifier.otherScopus: 84907946061
dc.identifier.otherORCID: /0000-0002-8863-7828/work/58531315
dc.identifier.otherWOS: 000344158500139
dc.descriptionFunding for WASP comes from consortium universities and from the UK’s Science and Technology Facilities Council (STFC).en
dc.description.abstractWe 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.relation.ispartofAstronomy & Astrophysicsen
dc.rightsReproduced with permission from Astronomy & Astrophysics, © ESOen
dc.subjectPlanets and satellites: detectionen
dc.subjectPlanets and satellites: fundamental parametersen
dc.subjectStars: individual: WASP-104ben
dc.subjectStars: individual: WASP-106ben
dc.subjectPlanetary systemsen
dc.subjectQB Astronomyen
dc.subjectQC Physicsen
dc.titleWASP-104b and WASP-106b : two transiting hot Jupiters in 1.75-day and 9.3-day orbitsen
dc.typeJournal articleen
dc.contributor.sponsorScience & Technology Facilities Councilen
dc.contributor.sponsorScience & Technology Facilities Councilen
dc.description.versionPublisher PDFen
dc.contributor.institutionUniversity of St Andrews. School of Physics and Astronomyen
dc.description.statusPeer revieweden

This item appears in the following Collection(s)

Show simple item record