Volume 499, Number 2, May IV 2009
|Page(s)||623 - 625|
|Section||Planets and planetary systems|
|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
Laboratoire d'Astrophysique de Grenoble, UMR5571 CNRS, Université Joseph Fourier, BP 53, 38041 Grenoble Cedex 9, France e-mail: firstname.lastname@example.org
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
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