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dc.contributor.authorWittenmyer, Robert A.
dc.contributor.authorHorner, Jonathan
dc.contributor.authorTinney, C. G.
dc.contributor.authorButler, R. P.
dc.contributor.authorJones, H. R A
dc.contributor.authorSalter, G. S.
dc.contributor.authorCarter, B. D.
dc.contributor.authorKoch, F. Elliott
dc.contributor.authorO'Toole, S. J.
dc.contributor.authorBailey, J.
dc.contributor.authorWright, D.
dc.contributor.authorTuomi, Mikko
dc.date.accessioned2017-03-09T17:42:01Z
dc.date.available2017-03-09T17:42:01Z
dc.date.issued2014-03-10
dc.identifier.citationWittenmyer , R A , Horner , J , Tinney , C G , Butler , R P , Jones , H R A , Salter , G S , Carter , B D , Koch , F E , O'Toole , S J , Bailey , J , Wright , D & Tuomi , M 2014 , ' The Anglo-Australian planet search. XXIII. Two new jupiter analogs ' , The Astrophysical Journal , vol. 783 , no. 2 , 103 . https://doi.org/10.1088/0004-637X/783/2/103
dc.identifier.issn0004-637X
dc.identifier.otherPURE: 11264677
dc.identifier.otherPURE UUID: 3beb6f47-3cf4-4938-b052-f870d5aac920
dc.identifier.otherScopus: 84896798249
dc.identifier.urihttp://hdl.handle.net/2299/17709
dc.descriptionRobert A. Wittenmyer, et al, 'The Anglo-Australian planet search. XXIII. Two new Jupiter analogs', The Astrophysical Journal, Vol. 783:103 (9pp), first published online 20 February 2014. The version of record is available online at doi:10.1088/0004-637X/783/2/103 © 2014. The American Astronomical Society. All rights reserved.
dc.description.abstractWe report the discovery of two long-period giant planets from the Anglo-Australian Planet Search. HD 154857c is in a multiple-planet system, while HD 114613b appears to be solitary. HD 114613b has an orbital period P = 10.5 yr, and a minimum mass msin i of 0.48 M Jup HD 154857c has P = 9.5 yr and msin i = 2.6 M Jup. These new data confirm the planetary nature of the previously unconstrained long-period object in the HD 154857 system. We have performed detailed dynamical stability simulations which show that the HD 154857 two-planet system is stable on timescales of at least 108 yr. These results highlight the continued importance of "legacy" surveys with long observational baselines; these ongoing campaigns are critical for determining the population of Jupiter analogs, and hence of those planetary systems with architectures most like our own solar system.en
dc.language.isoeng
dc.relation.ispartofThe Astrophysical Journal
dc.subjectplanets and satellites: detection
dc.subjectplanets and satellites: dynamical evolution and stability
dc.subjectplanets and satellites: individual (HD 114613, HD 154857)
dc.subjecttechniques: radial velocities
dc.subjectSpace and Planetary Science
dc.subjectAstronomy and Astrophysics
dc.subjectNuclear and High Energy Physics
dc.titleThe Anglo-Australian planet search. XXIII. Two new jupiter analogsen
dc.contributor.institutionCentre for Astrophysics Research
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.contributor.institutionScience & Technology Research Institute
dc.description.statusPeer reviewed
dc.identifier.urlhttp://www.scopus.com/inward/record.url?scp=84896798249&partnerID=8YFLogxK
rioxxterms.versionVoR
rioxxterms.versionofrecordhttps://doi.org/10.1088/0004-637X/783/2/103
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue


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