DOI: 10.1051/0004-6361/200809366e
Erratum
AGB stars as tracers of metallicity and mean age across M 33
M.-R. L. Cioni1, 2, M. Irwin3, A. M. N. Ferguson1, A. McConnachie4, B. C. Conn5, A. Huxor1, 6, R. Ibata7, G. Lewis8, and N. Tanvir91 SUPA, School of Physics, University of Edinburgh, IfA, Blackford Hill, Edinburgh EH9 3HJ, UK
2 Centre for Astrophysics Research, University of Hertfordshire, Hatfield AL10 9AB, UK
3 Institute of Astronomy, University of Cambridge, Madingley Road, Cambridge CB3 0HA, UK
4 Deptartment of Physics & Astronomy, University of Victoria, PO Box 3055, STN CSC, Victoria, BC, V8W 3P6 Canada
5 European Southern Observatory, Alonso de Cordova 3107, Vitacura, Santiago, Chile
6 Department of Physics, University of Bristol, Tyndall Avenue, Bristol BS8 1TL, UK
7 Observatoire de Strasbourg, 11 rue de l'Université, 67000 Strasbourg, France
8 Institute of Astronomy, School of Physics, A29, University of Sydney, NSW 2006, Australia
9 Department of Physics and Astronomy, University of Leicester, Leicester LE1 7RH, UK
Key words: galaxies: individual: M 33 -- stars: late-type -- galaxies: stellar content -- galaxy: abundances -- galaxies: structure -- errata, addenda
© ESO 2009

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