Files in this item
In the shadows of giants : a tomographic method for analysing the orbits of transiting exoplanets
Item metadata
dc.contributor.advisor | Cameron, A. C. | |
dc.contributor.author | Miller, Grant Robert MacKinnon | |
dc.coverage.spatial | 140 | en_US |
dc.date.accessioned | 2013-06-19T15:54:10Z | |
dc.date.available | 2013-06-19T15:54:10Z | |
dc.date.issued | 2013-06-26 | |
dc.identifier.uri | https://hdl.handle.net/10023/3735 | |
dc.description.abstract | The radial velocity anomaly which affects spectroscopic observations of stars undergoing transit by a companion body is known as the Rossiter-McLaughlin effect. This effect can be used to measure the obliquities of the orbits of transiting planets. In this thesis I present a tomographic method for analysing the effect, which manifests itself in stellar spectral line-profiles. I implement this method on seven systems known to host transiting planets, and some systems with early-type host stars, for which the transit events have not yet been shown to be the result of planetary companions. Despite being well-suited to examining systems with early-type, rapidly-rotating host stars which have a more pronounced Rossiter-McLaughlin effect, I find the tomographic method is able to produce reasonable results for the system parameters of planets orbiting relatively slowly-rotating stars. I show that the method provides a significant increase in the accuracy of determinations of the stellar rotation rate and is able to better constrain values for the transit impact parameter. Though I do not confirm the existence of any new planets around early-type stars, I do use the tomographic method to reject one candidate as a stellar eclipsing binary system, and also reveal that one of the candidate host stars is a non-radial pulsator. I show that the method is able to examine systems involving stars with a range of spectral types and rotation rates. | en_US |
dc.language.iso | en | en_US |
dc.publisher | University of St Andrews | |
dc.subject | Exoplanet | en_US |
dc.subject | Rossiter-McLaughlin | en_US |
dc.subject | Transiting | en_US |
dc.subject | Doppler tomography | en_US |
dc.subject | WASP | en_US |
dc.subject | Misalignment | en_US |
dc.subject.lcc | QB603.M6M5 | |
dc.subject.lcsh | Planets--Orbits--Measurement | en_US |
dc.subject.lcsh | Planets--Spectra--Measurement | en_US |
dc.subject.lcsh | Stars--Motion in line of sight | en_US |
dc.subject.lcsh | Astronomy--Methodology | en_US |
dc.title | In the shadows of giants : a tomographic method for analysing the orbits of transiting exoplanets | en_US |
dc.type | Thesis | en_US |
dc.type.qualificationlevel | Doctoral | en_US |
dc.type.qualificationname | PhD Doctor of Philosophy | en_US |
dc.publisher.institution | The University of St Andrews | en_US |
This item appears in the following Collection(s)
Items in the St Andrews Research Repository are protected by copyright, with all rights reserved, unless otherwise indicated.