dc.contributor.author | Jones, H.R.A. | |
dc.contributor.author | Butler, R.P. | |
dc.contributor.author | Tinney, C.G. | |
dc.contributor.author | Marcy, G.W. | |
dc.contributor.author | Carter, B.D. | |
dc.contributor.author | Penny, A.J. | |
dc.contributor.author | McCarthy, C. | |
dc.contributor.author | Bailey, J. | |
dc.date.accessioned | 2007-07-08T20:22:19Z | |
dc.date.available | 2007-07-08T20:22:19Z | |
dc.date.issued | 2006 | |
dc.identifier.citation | Jones , H R A , Butler , R P , Tinney , C G , Marcy , G W , Carter , B D , Penny , A J , McCarthy , C & Bailey , J 2006 , ' High-eccentricity planets from the Anglo-Australian planet search ' , Monthly Notices of the Royal Astronomical Society , vol. 369 , no. 1 , pp. 249-256 . | |
dc.identifier.issn | 0035-8711 | |
dc.identifier.other | PURE: 172605 | |
dc.identifier.other | PURE UUID: fc2da140-130b-4c25-9b9a-14f16c858453 | |
dc.identifier.other | dspace: 2299/179 | |
dc.identifier.other | Scopus: 33745263905 | |
dc.identifier.uri | http://hdl.handle.net/2299/179 | |
dc.description | The definitive version is available at www.blackwell-synergy.com--Copyright Blackwell Publishing | |
dc.description.abstract | We report Doppler measurements of the stars HD 187085 and HD 20782 which indi- cate two high eccentricity low-mass companions to the stars. We find HD 187085 has a Jupiter-mass companion with a 1000 d orbit. Our formal ‘best fit’ solution suggests an eccentricity of 0.47, however, it does not sample the periastron passage of the com- panion and we find that orbital solutions with eccentricities between 0.1 and 0.8 give only slightly poorer fits (based on RMS and 2 ) and are thus plausible. Observations made during periastron passage in 2007 June should allow for the reliable determi- nation of the orbital eccentricity for the companion to HD 187085. Our dataset for HD 20782 does sample periastron and so the orbit for its companion can be more reli- ably determined. We find the companion to HD 20782 has M sin i = 1.77±0.22 MJup, an orbital period of 595.86±0.03 d and an orbit with an eccentricity of 0.92±0.03. The detection of such high-eccentricity (and relatively low velocity amplitude) exoplanets appears to be facilitated by the long-term precision of the Anglo-Australian Planet Search. Looking at exoplanet detections as a whole, we find that those with higher eccentricity seem to have relatively higher velocity amplitudes indicating higher mass planets and/or an observational bias against the detection of high eccentricity systems. | en |
dc.language.iso | eng | |
dc.relation.ispartof | Monthly Notices of the Royal Astronomical Society | |
dc.title | High-eccentricity planets from the Anglo-Australian planet search | en |
dc.contributor.institution | School of Physics, Astronomy and Mathematics | |
dc.contributor.institution | Science & Technology Research Institute | |
dc.contributor.institution | Centre for Astrophysics Research | |
dc.description.status | Peer reviewed | |
rioxxterms.type | Journal Article/Review | |
herts.preservation.rarelyaccessed | true | |