| Issue |
A&A
Volume 684, April 2024
|
|
|---|---|---|
| Article Number | C1 | |
| Number of page(s) | 1 | |
| Section | Interstellar and circumstellar matter | |
| DOI | https://doi.org/10.1051/0004-6361/202449494e | |
| Published online | 01 April 2024 | |
H I filaments are cold and associated with dark molecular gas
HI4PI-based estimates of the local diffuse CO-dark H2 distribution (Corrigendum)★
1
Argelander-Institut für Astronomie,
Auf dem Hügel 71,
53121
Bonn,
Germany
e-mail: pkalberla@astro.uni-bonn.de
2
Tartu Observatory, University of Tartu,
61602
Tõravere,
Tartumaa,
Estonia
This article has no abstract.
Key words: ISM: clouds / ISM: structure / ISM: molecules / dust, extinction / errata, addenda
Corrected FITS files are available at the CDS via anonymous ftp to cdsarc.cds.unistra.fr (130.79.128.5) or via https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/639/A26
© The Authors 2024
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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