Volume 390, Number 1, July IV 2002
|Page(s)||267 - 279|
|Published online||05 July 2002|
The CORALIE survey for southern extra-solar planets*
VIII. The very low-mass companions of HD 141937, HD 162020, HD 168443 and HD 202206: Brown dwarfs or “superplanets”?
Observatoire de Genève, 51 ch. des Maillettes, 1290 Sauverny, Switzerland
Corresponding author: S. Udry, firstname.lastname@example.org
Accepted: 22 April 2002
Doppler CORALIE measurements of the solar-type stars HD 141937, HD 162020, HD 168443 and HD 202206 show Keplerian radial-velocity variations revealing the presence of 4 new companions with minimum masses close to the planet/brown-dwarf transition, namely with 9.7, 14.4, 16.9, and 17.5 MJup, respectively. The orbits present fairly large eccentricities (). Except for HD 162020, the parent stars are metal rich compared to the Sun, as are most of the detected extra-solar planet hosts. Considerations of tidal dissipation in the short-period HD 162020 system points towards a brown-dwarf nature for the low-mass companion. HD 168443 is a multiple system with two low-mass companions being either brown dwarfs or formed simultaneously in the protoplanetary disks as superplanets. For HD 202206, the radial velocities show an additional drift revealing a further outer companion, the nature of which is still unknown. Finally, the stellar-host and orbital properties of massive planets are examined in comparison to lighter exoplanets. Observed trends include the need of metal-rich stars to form massive exoplanets and the lack of short periods for massive planets. If confirmed with improved statistics, these features may provide constraints for the migration scenario.
Key words: techniques: radial velocities / stars: binaries: spectroscopic / stars: individual: HD 141937 / stars: individual: HD 162020 / stars: individual: HD 168443 / stars: individual: HD 202206
© ESO, 2002
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