Abstract
We report the detection of a new candidate exoplanet around the metal- rich star 1 Gruis. With M sin i = 1.23±0.18 MJUP, a period of 1326±300 d and an orbit with an eccentricity of 0.14±0.14 it adds to the growing popula- tion of long period exoplanets with near-circular orbits. This population now comprises more than 20% of known exoplanets.
Original language | English |
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Pages (from-to) | 948-952 |
Journal | Monthly Notices of the Royal Astronomical Society (MNRAS) |
Volume | 341 |
Issue number | 3 |
Publication status | Published - May 2003 |