Journal
ASTRONOMY & ASTROPHYSICS
Volume 444, Issue 2, Pages L21-L24Publisher
EDP SCIENCES S A
DOI: 10.1051/0004-6361:200500176
Keywords
techniques : radial velocities; stars : binaries : spectroscopic; stars : early type; stars : brown dwarfs; planetary systems
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We present here the detection of a planet orbiting around the F6V star HD33564. The radial velocity measurments, obtained with the ELODIE , echelle spectrograph at the Haute-Provence Observatory, show a variation with a period of 388 days. Assuming a primary mass of 1.25 M-circle dot, the, best Keplerian fit to the data leads to a minimum mass of 9.1 M-Jup for the companion.
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