Distorted, non-spherical transiting planets: impact on the transit depth and on the radius determination (Corrigendum)

Free access article

This article is an erratum for: [this article]

Issue		A&A Volume 536, December 2011


Article Number		C1
Number of page(s)		2
Section		Planets and planetary systems
DOI		http://dx.doi.org/10.1051/0004-6361/201015811e
Published online		19 December 2011

A&A 536, C1 (2011)

Distorted, non-spherical transiting planets: impact on the transit depth and on the radius determination (Corrigendum)

J. Leconte¹^,4, D. Lai²^,4 and G. Chabrier¹^,3^,4

¹ École normale supérieure de Lyon, CRAL (CNRS), 46 allée d’Italie, 69007 Lyon, Université de Lyon, France
e-mail: jeremy.leconte@ens-lyon.fr; chabrier@ens-lyon.fr
² Center for Space Research, Department of Astronomy, Cornell University, Ithaca, NY 14853, USA
e-mail: dong@astro.cornell.edu
³ School of Physics, University of Exeter, Exeter, UK
⁴ KITP, University of Santa Barbara, USA

This article has no abstract.

Key words: planets and satellites: interiors / planets and satellites: fundamental parameters / planets and satellites: general / errata, addenda / equation of state

Erratum of: A&A 528, A41 (2011)

© ESO, 2011

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