A bright early-type star in the halo of NGC 253: Runaway or in situ formation?

F. Comerón; A. E. Gómez; J. Torra

doi:10.1051/0004-6361:20030311

Free Access

Erratum

This article is an erratum for: [this article]

Issue		A&A Volume 402, Number 1, April IV 2003


Page(s)		181 - 181
Section		Extragalactic astronomy
DOI		https://doi.org/10.1051/0004-6361:20030311
Published online		07 April 2003

A&A 402, 181-181 (2003)

A bright early-type star in the halo of NGC 253: Runaway or in situ formation?

F. Comerón¹, A. E. Gómez² and J. Torra³

¹ European Southern Observatory, Karl-Schwarzschild-Strasse 2, 85748 Garching bei Muenchen, Germany e-mail: fcomeron@eso.org
² Observatoire de Paris-Meudon, DASGAL, UMR 8633 du CNRS, 92195 Meudon Cedex, France e-mail: ana.gomez@obspm.fr
³ Departament d'Astronomia i Meteorologia, Universitat de Barcelona, Av. Diagonal 647, 08028 Barcelona, Spain e-mail: jordi@am.ub.es

Corresponding author: F. Comerón, fcomeron@eso.org

This article has no abstract.

Key words: errata, addenda / galaxies: individual: NGC 253 / galaxies: starburst / stars: early-type / stars: formation / stars: kinematics

Erratum to: A&A, 400, 137–143 (2003), DOI: 10.1051/0004-6361:20021909

© ESO, 2003

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