The AMIGA sample of isolated galaxies (Corrigendum)

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This article is an erratum for: [this article]

Issue		A&A Volume 538, February 2012


Article Number		C1
Number of page(s)		1
Section		Extragalactic astronomy
DOI		http://dx.doi.org/10.1051/0004-6361/201117056e
Published online		08 February 2012

A&A 538, C1 (2012)

IX. Molecular gas properties

U. Lisenfeld¹^,2, D. Espada³^,4, L. Verdes-Montenegro³, N. Kuno⁵, S. Leon⁶, J. Sabater⁷, N. Sato⁸, J. Sulentic³, S. Verley¹ and M. S. Yun⁹

¹ Departamento de Física Teórica y del Cosmos, Universidad de Granada, 18071 Granada, Spain
e-mail: ute@ugr.es
² Instituto Carlos I de Física Teórica y Computacional, Universidad de Granada, Spain
³ Instituto de Astrofísica de Andalucía (CSIC) Apdo. 3004, 18080 Granada, Spain
⁴ National Astronomical Observatory of Japan, 2-21-1 Osawa, Mitaka, Tokyo 181-8588, Japan
⁵ Nobeyama Radio Observatory, Minamimaki, Minamisaku, Nagano 384-1805, Japan
⁶ Joint Alma Observatory/ESO, Las Condes, Santiago, Chile
⁷ Institute for Astronomy, University of Edinburgh, Edinburgh EH9 3HJ, UK
⁸ Student Center for Independent Research in the Science, Wakayama University, 930 Sakaedani, Wakayama, 640-8510, Japan
⁹ Department of Astronomy, University of Massachusetts, Amherst, MA 01003, USA

This article has no abstract.

Key words: galaxies: evolution / galaxies: ISM / galaxies: interactions / radio lines: ISM / radio lines: galaxies / errata, addenda

Erratum of: A&A 534, A102 (2011), DOI: 10.1051/0004-6361/201117056

© ESO, 2012

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