Issue |
A&A
Volume 562, February 2014
|
|
---|---|---|
Article Number | C1 | |
Number of page(s) | 2 | |
Section | Letters | |
DOI | https://doi.org/10.1051/0004-6361/201116631e | |
Published online | 31 January 2014 |
Deuteration as an evolutionary tracer in massive-star formation (Corrigendum)⋆,⋆⋆
1 INAF – Osservatorio Astrofisico di Arcetri, L.go E. Fermi 5, 50125 Firenze, Italy
e-mail: fontani@arcetri.astro.it
2 Institut de Ciències de l’Espai (CSIC-IEEC), Campus UAB-Facultat de Ciències, Torre C5-parell 2, 08193 Bellaterra, Spain
3 School of Physics and Astronomy, E.C. Stoner Building, University of Leeds, Leeds LS2 9JT, UK
4 I. Physikalisches Institut der Universitat zu Köln, Zülpic her Str. 77, 50937 Köln, Germany
5 Department of Astronomy, University of Florida, Gainesville, 32611, USA
6 Department of Physics, University of Florida, Gainesville, 32611, USA
7 European Southern Observatory, Karl-Schwarzschild-Str. 2, 85748 Garching, Germany
8 Max-Planck-Institut für Radioastronomie, Auf dem Hügel 69, 53121 Bonn, Germany
9 ISDC Data Center for Astrophysics, University of Geneva, Ch. d’Ecogia 16, 1290 Versoix, Switzerland
10 Geneva Observatory, University of Geneva, ch. des Maillettes 51, 1290 Versoix, Switzerland
This article has no abstract.
Key words: stars: formation / radio lines: ISM / ISM: clouds / ISM: molecules / errata, addenda
Based on observations carried out with the IRAM 30 m telescope. IRAM is supported by INSU/CNRS (France), MPG (Germany), and IGN (Spain).
Table 1 is available in electronic form at http://www.aanda.org
© ESO, 2014
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