[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.
This article is published in open access under the Subscribe to Open model.
Open access funding provided by Max Planck Society.
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.