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dc.contributor.authorTriaud, Amaury
dc.contributor.authorCollier Cameron, Andrew
dc.contributor.authorQueloz, Didier
dc.contributor.authorAnderson, David
dc.contributor.authorBrown, David John Alexander
dc.contributor.authorSmalley, Barry
dc.contributor.authorBouchy, Francois
dc.contributor.authorLendl, Monika
dc.contributor.authorGillon, Michael
dc.date.accessioned2014-08-14T14:31:01Z
dc.date.available2014-08-14T14:31:01Z
dc.date.issued2013-07-01
dc.identifier.citationTriaud , A , Collier Cameron , A , Queloz , D , Anderson , D , Brown , D J A , Smalley , B , Bouchy , F , Lendl , M & Gillon , M 2013 , ' Spin-orbit angles as a probe to orbital evolution ' , Protostars and Planets VI , Heidelberg , Germany , 15/07/13 - 20/07/13 . https://doi.org/10.1017/S174392131300759Xen
dc.identifier.citationconferenceen
dc.identifier.otherPURE: 140357911
dc.identifier.otherPURE UUID: 2a211768-3de6-4ac8-8fe6-f09da6091ed0
dc.identifier.otherBibCode: 2013prpl.conf2H037T
dc.identifier.otherScopus: 84891879444
dc.identifier.otherORCID: /0000-0002-8863-7828/work/58531510
dc.identifier.urihttps://hdl.handle.net/10023/5161
dc.description.abstractThe WASP (Wide Angle Search for Planets) has discovered 75 planets in the Southern Hemisphere. We followed-up 40 of these and observed the Rossiter-McLaughlin effect. It allows us to measure the angle between the stellar spin and the planet's orbital spin. Here, we present the results of our survey, along with results published in the literature.Our observations reveal a wide distribution in orbital angle, indicative or past dynamical interactions. Our data also demonstrates the important effects that tidal interactions have in altering the spin-orbitdistribution. This renders any interpretation tricky. However, comparing different sub-samples we start uncovering evidence that two types of migration are maybe acting to create the hot Jupiter population.
dc.language.isoeng
dc.rightsCopyright 2013, authorsen
dc.subjectQB Astronomyen
dc.subject.lccQBen
dc.titleSpin-orbit angles as a probe to orbital evolutionen
dc.typeConference posteren
dc.contributor.sponsorScience & Technology Facilities Councilen
dc.contributor.sponsorScience & Technology Facilities Councilen
dc.description.versionPostprinten
dc.contributor.institutionUniversity of St Andrews. School of Physics and Astronomyen
dc.identifier.doihttps://doi.org/10.1017/S174392131300759X
dc.description.statusPeer revieweden
dc.identifier.urlhttp://adsabs.harvard.edu/abs/2013prpl.conf2H037Ten
dc.identifier.grantnumberST/J001651/1en
dc.identifier.grantnumberPP/F000065/1en


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