Herschel CHESS discovery of the fossil cloud that gave birth to the Trapezium and Orion KL (Corrigendum)

A. López-Sepulcre; M. Kama; C. Ceccarelli; C. Dominik; E. Caux; A. Fuente; T. Alonso-Albi

doi:10.1051/0004-6361/201219416e

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Erratum

This article is an erratum for:
[https://doi.org/10.1051/0004-6361/201219416]

Issue		A&A Volume 553, May 2013


Article Number		C1
Number of page(s)		1
Section		Interstellar and circumstellar matter
DOI		https://doi.org/10.1051/0004-6361/201219416e
Published online		17 May 2013

A&A 553, C1 (2013)

Herschel CHESS discovery of the fossil cloud that gave birth to the Trapezium and Orion KL (Corrigendum)

A. López-Sepulcre¹, M. Kama², C. Ceccarelli¹, C. Dominik²^,3, E. Caux⁴^,5, A. Fuente⁶ and T. Alonso-Albi⁶

¹ UJF-Grenoble 1/CNRS-INSU, Institut de Planétologie et d’Astrophysique de Grenoble (IPAG) UMR 5274, 38041 Grenoble, France
e-mail: ana.sepulcre@obs.ujf-grenoble.fr
² Astronomical Institute Anton Pannekoek, University of Amsterdam, Amsterdam, The Netherlands
³ Department of Astrophysics/IMAPP, Radboud University Nijmegen, Nijmegen, The Netherlands
⁴ Université de Toulouse, UPS-OMP, IRAP, Toulouse, France
⁵ CNRS, IRAP, 9 Av. colonel Roche, BP 44346, 31028 Toulouse Cedex 4, France
⁶ Observatorio Astronómico Nacional, PO Box 112, 28803 Alcalá de Henares, Madrid, Spain

Key words: astrochemistry / ISM: abundances / ISM: molecules / ISM: clouds / photon-dominated region (PDR) / errata, addenda

Erratum for: A&A 549, A114 (2013), DOI: 10.1051/0004-6361/201219416

An error occurred during the production process. The right panel of Fig. 1 was the same as the left one. The correct Fig. 1 is shown here.

Fig. 1

Spectral lines detected in absorption towards OMC-2 FIR 4. The green vertical lines mark V_LSR = 9.3 km s^-1, i.e. the systemic velocity of the OH⁺ lines.

© ESO, 2013

All Figures

	Fig. 1 Spectral lines detected in absorption towards OMC-2 FIR 4. The green vertical lines mark V_LSR = 9.3 km s^-1, i.e. the systemic velocity of the OH⁺ lines.
In the text

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