A search for multi-planet systems

dc.contributor.advisorCochran, William D.en
dc.creatorWittenmyer, Robert Andrew, 1976-en
dc.date.accessioned2012-09-07T18:26:05Zen
dc.date.accessioned2017-05-11T22:27:20Z
dc.date.available2012-09-07T18:26:05Zen
dc.date.available2017-05-11T22:27:20Z
dc.date.issued2008-05en
dc.descriptiontexten
dc.description.abstractI report the results of a three-year intensive radial-velocity survey of 22 planet-host stars in search of the low-amplitude (K ~5-10 m s⁻¹) signals from additional planets which may be "hiding" in the residuals of the known planet orbital solution. On average, more than 40 radial-velocity observations were obtained for each target using the High-Resolution Spectrograph at the 9.2m Hobby-Eberly Telescope (HET). These high-precision data can be used to rule out additional planets in some of these systems to a detection limit of M sin i ~10-20 Earth masses at a = 0:05 AU. Jupiter-mass planets can be excluded at the 99% level for orbital separations a < 2 AU. No additional planets are evident, and our data do not confirm the planets HD 20367b, HD 74156d, and 47 UMa c. Test particle simulations of these systems with the SWIFT N-body integrator reveal the regions where additional planets could reside in stable orbits. Further simulations with Saturn-mass bodies in these regions are also performed. We note a lack of short-period giant planets in any of these 22 systems, despite dynamical feasibility. The frequency of inner giant planets may be much lower than what was expected based on early discoveries of such objects in systems containing jovian-mass planets. Terrestrial-mass planets may be present in these systems but as yet undetectable. These results suggest that planet formation and migration processes do not favor systems containing both "hot" and "cold" Jupiters. Hence, as detection methods become sensitive to terrestrial-mass planets, systems with architectures like our own Solar system may yet be commonplace.en
dc.description.departmentAstronomyen
dc.format.mediumelectronicen
dc.identifier.urihttp://hdl.handle.net/2152/17826en
dc.language.isoengen
dc.rightsCopyright is held by the author. Presentation of this material on the Libraries' web site by University Libraries, The University of Texas at Austin was made possible under a limited license grant from the author who has retained all copyrights in the works.en
dc.subject.lcshStars with planetsen
dc.subject.lcshAstronomyen
dc.titleA search for multi-planet systemsen

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