[https://doi.org/10.1051/0004-6361/202039465]
[https://doi.org/10.1051/0004-6361/201833583]
| Issue |
A&A
Volume 672, April 2023
|
|
|---|---|---|
| Article Number | C1 | |
| Number of page(s) | 4 | |
| Section | Interstellar and circumstellar matter | |
| DOI | https://doi.org/10.1051/0004-6361/202039465e | |
| Published online | 28 March 2023 | |
Physical and chemical structure of the Serpens filament: Fast formation and gravity-driven accretion (Corrigendum)
1
Max-Planck-Institut für Radioastronomie,
Auf dem Hügel 69,
53121
Bonn, Germany
e-mail: ygong@mpifr-bonn.mpg.de; gongyan2444@gmail.com
2
Purple Mountain Observatory and Key Laboratory of Radio Astronomy, Chinese Academy of Sciences,
Nanjing
210034, PR China
3
Astronomy Department, Faculty of Science, King Abdulaziz University,
PO Box 80203,
Jeddah
21589, Saudi Arabia
4
South-Western Institute for Astronomy Research, Yunnan University,
Kunming,
650500
Yunnan, PR China
This article has no abstract.
Key words: ISM: clouds / ISM: individual objects: the Serpens filament / radio lines: ISM / ISM: kinematics and dynamics / ISM: molecules / errata / addenda
© The Authors 2023
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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Open access funding provided by Max Planck Society.
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