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This article is an erratum for: [this article]

Issue A&A
Volume 499, Number 2, May IV 2009
Page(s) 623 - 625
Section Planets and planetary systems
DOI http://dx.doi.org/10.1051/0004-6361/200810241e
Published online 16 April 2009

A&A 499, 623-625 (2009)
DOI: 10.1051/0004-6361/200810241e

Erratum

Extrasolar planets and brown dwarfs around A–F type stars

V. A planetary system found with HARPS around the F6IV–V star HD 60532
M. Desort1, A.-M. Lagrange1, F. Galland1, H. Beust1, S. Udry2, M. Mayor2, and G. Lo Curto3

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

Abstract
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, $\Omega_c-\Omega_b$ 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]$_{\rm updated}$ = -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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