| Issue |
A&A
Volume 568, August 2014
|
|
|---|---|---|
| Article Number | C1 | |
| Number of page(s) | 3 | |
| Section | Interstellar and circumstellar matter | |
| DOI | https://doi.org/10.1051/0004-6361/201323293e | |
| Published online | 28 August 2014 | |
Herschel-Planck dust optical-depth and column-density maps (Corrigendum)
I. Method description and results for Orion
1 University of Milan, Department of Physics, via Celoria 16, 20133 Milan, Italy
e-mail: marco.lombardi@unimi.it
2 Centro de Astrobiología, INTA-CSIC, PO Box 78, 28691 Villanueva de la Cañada, Madrid, Spain
3 University of Vienna, Türkenschanzstrasse 17, 1180 Vienna, Austria
4 Harvard-Smithsonian Center for Astrophysics, Mail Stop 72, 60 Garden Street, Cambridge, MA 02138, USA
This article has no abstract.
Key words: ISM: clouds / dust, extinction / ISM: structure / ISM: individual objects: Orion molecular cloud / errata, addenda
© ESO, 2014
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