| Issue |
A&A
Volume 712, August 2026
|
|
|---|---|---|
| Article Number | C3 | |
| Number of page(s) | 2 | |
| Section | Interstellar and circumstellar matter | |
| DOI | https://doi.org/10.1051/0004-6361/202661829e | |
| Published online | 30 July 2026 | |
A molecule-rich torus-like structure in the 21 μm source IRAS 23304+6147 (Corrigendum)
1
School of Physics and Astronomy, Sun Yat-sen University,
2 Daxue Road, Tangjia, Zhuhai
519082,
Guangdong Province,
China
2
Xinjiang Astronomical Observatory, Chinese Academy of Sciences,
150 Science 1-Street,
Urumqi
830011,
China
3
CSST Science Center for the Guangdong-Hongkong-Macau Greater Bay Area, Sun Yat-Sen University,
Guangdong Province,
China
4
School of physics and astronomy, Yunnan University,
Kunming
650091,
China
5
School of Mathematics and Physics, Jinggangshan University,
28 Xueyuan Road, Qingyuan District, Ji’an
343009,
Jiangxi Province,
China
6
Xinjiang Key Laboratory of Radio Astrophysics,
150 Science 1-Street, Urumqi,
Xinjiang
830011,
China
7
Key Laboratory of Radio Astronomy and Technology, Chinese Academy of Sciences,
A20 Datun Road, Chaoyang District,
Beijing,
100101,
China
★ Corresponding author: This email address is being protected from spambots. You need JavaScript enabled to view it.
This article has no abstract.
Key words: stars: AGB and post-AGB / circumstellar matter / ISM: molecules / planetary nebulae: general / radio lines: ISM / errata, addenda
© The Authors 2026
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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