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dc.contributor.authorJones, H.R.A.
dc.contributor.authorButler, R.P.
dc.contributor.authorTinney, C.G.
dc.contributor.authorMarcy, G.W.
dc.contributor.authorPenny, A.J.
dc.contributor.authorMcCarthy, C.
dc.contributor.authorPourbaix, D.
dc.date.accessioned2007-07-08T20:22:16Z
dc.date.available2007-07-08T20:22:16Z
dc.date.issued2002-07
dc.identifier.citationJones , H R A , Butler , R P , Tinney , C G , Marcy , G W , Penny , A J , McCarthy , C & Pourbaix , D 2002 , ' A probable planetary companion to HD 39091 from the Anglo-Australian Planet Search ' , Monthly Notices of the Royal Astronomical Society , vol. 333 , no. 4 , pp. 871-875 .
dc.identifier.issn0035-8711
dc.identifier.otherPURE: 166862
dc.identifier.otherPURE UUID: 5a65b58d-5401-4621-8adf-218ba6b4dc14
dc.identifier.otherdspace: 2299/175
dc.identifier.otherScopus: 0000120551
dc.identifier.urihttp://hdl.handle.net/2299/175
dc.description.abstractWe report the detection of a extrasolar planet candidate orbiting the G1 V star HD 39091. The orbital period is 2083 d and the eccentricity is 0.62. With a minimum (M sin i) mass of 10.3 MJUP this object falls near the high mass end of the observed planet mass function, and may plausibly be a brown dwarf. Other characteristics of this system, including orbital eccentricity and metallicity, are typical of the well populated class of radial velocity planets in eccentric orbits around metal-rich stars.en
dc.language.isoeng
dc.relation.ispartofMonthly Notices of the Royal Astronomical Society
dc.rightsOpen
dc.titleA probable planetary companion to HD 39091 from the Anglo-Australian Planet Searchen
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.description.statusPeer reviewed
dc.relation.schoolSchool of Physics, Astronomy and Mathematics
dcterms.dateAccepted2002-07
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue
herts.rights.accesstypeOpen


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