Issue |
A&A
Volume 499, Number 2, May IV 2009
|
|
---|---|---|
Page(s) | 623 - 625 | |
Section | Planets and planetary systems | |
DOI | https://doi.org/10.1051/0004-6361/200810241e | |
Published online | 16 April 2009 |
Extrasolar planets and brown dwarfs around A–F type stars
V. A planetary system found with HARPS around the F6IV–V star HD 60532
1
Laboratoire d'Astrophysique de Grenoble, UMR5571 CNRS, Université Joseph Fourier, BP 53, 38041 Grenoble Cedex 9, France e-mail: mdesort@obs.ujf-grenoble.fr
2
Observatoire de Genève, Université de Genève, 51 chemin des Maillettes, 1290 Sauverny, Switzerland
3
European Southern Observatory, Alonso de Cordova 3107, Vitacura, Santiago, Chile
The dynamical analysis in the original paper was erroneous due to a
mismatch in the choice of angular parameters. The calculations had been made
by assuming a pole-on (sin i = 0) instead of an edge-on sin i = 1
orbit. In this framework, is just the mutual
inclination between the orbital planes of the two planets. We also
correct some stellar parameters given in the original paper (log g = +3.83, [Fe/H]updated = -0.26 ).
Key words: techniques: radial velocities / stars: early-type / stars: planetary systems / stars: oscillations / individual: HD 60532 / errata, addenda
© ESO, 2009
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.