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dc.contributor.authorMcCarthy, C.
dc.contributor.authorJones, H.R.A.
dc.contributor.authorButler, R.P.
dc.contributor.authorCarter, B.D.
dc.contributor.authorMarcy, G.W.
dc.contributor.authorPenny, A.J.
dc.contributor.authorBlundell, J.
dc.contributor.authorBond, J.
dc.date.accessioned2007-07-08T20:22:16Z
dc.date.available2007-07-08T20:22:16Z
dc.date.issued2003
dc.identifier.citationMcCarthy , C , Jones , H R A , Butler , R P , Carter , B D , Marcy , G W , Penny , A J , Blundell , J & Bond , J 2003 , Recent Discoveries from the Anglo-Australian Planet Search . in . Scientific Frontiers in Research on Extrasolar Planets, ASP Conference Series 294 . Astronomical Society of the Pacific , pp. 35-38 .
dc.identifier.isbn1-58381-141-9
dc.identifier.otherPURE: 171224
dc.identifier.otherPURE UUID: 099ebd9b-1701-4d6a-a889-61a910d531b5
dc.identifier.otherdspace: 2299/176
dc.identifier.urihttp://hdl.handle.net/2299/176
dc.descriptionOriginal paper can be found at: http://www.astrosociety.org/pubs/cs/confseries.html
dc.description.abstractWe present the latest precision radial velocity results from the Anglo Australian Planet Search. These include new planet mass companions to HD216437, HD196050, HD30177, HD73526, and HD2039, as well as evidence for a second companion to HD160691 residing in a long period orbit. The results come from a sample of ~ 200 nearby inactive FGKM dwarfs with V<7.5 and a subsample of 20 more distant metal rich stars. At least 25 ± 11% of metal rich stars appear to have planets within 2.5 AU, somewhat more than the 8% of stars which appear to have planets within 3.5 AU.en
dc.language.isoeng
dc.publisherAstronomical Society of the Pacific
dc.relation.ispartof. Scientific Frontiers in Research on Extrasolar Planets, ASP Conference Series 294
dc.titleRecent Discoveries from the Anglo-Australian Planet Searchen
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
rioxxterms.typeOther
herts.preservation.rarelyaccessedtrue


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