Issue |
A&A
Volume 663, July 2022
|
|
---|---|---|
Article Number | C1 | |
Number of page(s) | 2 | |
Section | Letters to the Editor | |
DOI | https://doi.org/10.1051/0004-6361/202142281e | |
Published online | 01 July 2022 |
Letter to the Editor
The width of Herschel filaments varies with distance (Corrigendum)
1
California Institute of Technology, Mail Code 350-17, 1200 E. California Blvd, Pasadena, CA 91125, USA
e-mail: panopg@caltech.edu
2
Department of Physics, Stanford University, Stanford, California 94305, USA
3
Kavli Institute for Particle Astrophysics & Cosmology, PO Box 2450 Stanford University, Stanford, CA 94305, USA
4
Department of Astrophysics, University of Vienna, Türkenschanzstrasse 17, 1180 Vienna, Austria
5
Department of Physics & Astronomy, University of North Carolina, Chapel Hill, North Carolina 27599, USA
6
Chalmers University of Technology, Department of Space, Earth and Environment, 412 93 Gothenburg, Sweden
7
Scuola Normale Superiore di Pisa, Piazza dei Cavalieri, 7, 56126 Pisa, Italy
8
University of Cologne, I. Physical Institute, Zülpicher Str. 77, 50937 Cologne, Germany
9
Jodrell Bank Centre for Astrophysics, Department of Physics and Astronomy, University of Manchester, Oxford Road, Manchester M13 9PL, UK
This article has no abstract.
Key words: ISM: clouds / ISM: structure / stars: formation / local insterstellar matter / errata, addenda
© G. V. Panopoulou et al. 2022
Open Access article, published by EDP Sciences, under the terms of the Creative Commons Attribution License (https://creativecommons.org/licenses/by/4.0), which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.
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