High eccentricity planets from the Anglo-Australian Planet Search

Hugh R. A. Jones; R. Paul Butler; C. G. Tinney; Geoffrey W. Marcy; Brad D. Carter; Alan J. Penny; Chris McCarthy; Jeremy Bailey

doi:10.1111/j.1365-2966.2006.10298.x

arXiv · astro-ph/0603335

High eccentricity planets from the Anglo-Australian Planet Search

Hugh R. A. Jones·R. Paul Butler·C. G. Tinney·Geoffrey W. Marcy·Brad D. Carter·Alan J. Penny·Chris McCarthy·Jeremy Bailey

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Abstract

We report Doppler measurements of the stars HD187085 and HD20782 which indicate two high eccentricity low-mass companions to the stars. We find HD187085 has a Jupiter-mass companion with a ~1000d orbit. Our formal `best fit' solution suggests an eccentricity of 0.47, however, it does not sample the periastron passage of the companion and we find that orbital solutions with eccentricities between 0.1 and 0.8 give only slightly poorer fits (based on RMS and chi^2) and are thus plausible. Observations made during periastron passage in 2007 June should allow for the reliable determination of the orbital eccentricity for the companion to HD187085. Our dataset for HD20782 does sample periastron and so the orbit for its companion can be more reliably determined. We find the companion to HD20782 has M sin i=1.77+/-0.22M_JUP, an orbital period of 595.86+/-0.03d 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.

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Hugh R. A. Jones, R. Paul Butler, C. G. Tinney, Geoffrey W. Marcy, Brad D. Carter, Alan J. Penny, Chris McCarthy, Jeremy Bailey. 2006-03-14. High eccentricity planets from the Anglo-Australian Planet Search. https://doi.org/10.1111/j.1365-2966.2006.10298.x

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