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dc.contributor.authorButler, R.P.
dc.contributor.authorTinney, C.G.
dc.contributor.authorMarcy, G.W.
dc.contributor.authorJones, H.R.A.
dc.contributor.authorPenny, A.J.
dc.contributor.authorApps, K.
dc.date.accessioned2007-07-04T15:10:06Z
dc.date.available2007-07-04T15:10:06Z
dc.date.issued2001-07
dc.identifier.citationButler , R P , Tinney , C G , Marcy , G W , Jones , H R A , Penny , A J & Apps , K 2001 , ' Two New Planets from the Anglo-Australian Planet Search ' , The Astrophysical Journal , vol. 555 , pp. 410-417 .
dc.identifier.issn0004-637X
dc.identifier.otherPURE: 172046
dc.identifier.otherPURE UUID: 162373a3-f908-4419-be8b-c9d05208b6f4
dc.identifier.otherdspace: 2299/137
dc.identifier.otherScopus: 0035402278
dc.identifier.urihttp://hdl.handle.net/2299/137
dc.descriptionOriginal article can be found at: http://www.journals.uchicago.edu/ Copyright The American Astronomical Society
dc.description.abstractPrecise Doppler measurements from the Anglo-Australian Telescope (AAT) UCLES spectrometer reveal periodic Keplerian velocity variations in the stars HD 160691 and HD 27442. HD 160691 has a period of 743 days, a semiamplitude of 54 m s~1, and a high eccentricity, e\0.62, typical of extrasolar planets orbiting beyond 0.2 AU. The minimum (M sin i) mass of the companion is 1.97 MJ and the , semimajor axis is 1.65 AU. HD 27442 has a 415 day period, a semiamplitude of 32 m s~1, and an eccentricity of 0.058. The minimum mass is 1.43 MJ and the semimajor axis is 1.18 AU. This is the first , extrasolar planet orbiting beyond 0.2 AU that is in a circular orbit similar to solar system planets. The photon-limited precision of AAT/UCLES measurements is 3 m s~1 as demonstrated by stable stars and Keplerian fits to planet-bearing stars. In addition, we present confirmation of four previously announced planets.en
dc.language.isoeng
dc.relation.ispartofThe Astrophysical Journal
dc.titleTwo New Planets from the Anglo-Australian Planet Searchen
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.contributor.institutionSchool of Physics, Engineering & Computer Science
dc.contributor.institutionDepartment of Physics, Astronomy and Mathematics
dc.contributor.institutionCentre of Data Innovation Research
dc.contributor.institutionCentre for Astrophysics Research
dc.description.statusPeer reviewed
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue


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