| Issue |
A&A
Volume 666, October 2022
|
|
|---|---|---|
| Article Number | C2 | |
| Number of page(s) | 1 | |
| Section | Interstellar and circumstellar matter | |
| DOI | https://doi.org/10.1051/0004-6361/201527364e | |
| Published online | 30 September 2022 | |
Dust emissivity in the star-forming filament OMC 2/3 (Corrigendum)
1
Max-Planck-Institut für Astronomie (MPIA),
Königstuhl 17,
69117
Heidelberg, Germany
e-mail: sarah.sadavoy@queensu.ca
2
National Radio Astronomy Observatory,
520 Edgemont Road,
Charlottesville,
VA 22903, USA
3
National Research Council Canada,
5071 West Saanich Road,
Victoria,
BC V9E 2E7, Canada
4
Department of Physics & Astronomy, University of Victoria,
PO Box 3055,
STN CSC,
Victoria,
BC V8W 3P6, Canada
5
Dunlap Institute for Astronomy and Astrophysics, University of Toronto,
50 St. George Street,
Toronto,
M5S 3H4
Ontario, Canada
This article has no abstract.
Key words: stars: formation / dust / extinction / ISM: clouds / submillimeter: ISM / errata / addenda
© S. I. Sadavoy 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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