| Issue |
A&A
Volume 692, December 2024
|
|
|---|---|---|
| Article Number | C4 | |
| Number of page(s) | 2 | |
| Section | Interstellar and circumstellar matter | |
| DOI | https://doi.org/10.1051/0004-6361/202452929e | |
| Published online | 13 December 2024 | |
CO emission survey of asymptotic giant branch stars with ultraviolet excesses (Corrigendum)
1
Centro de Astrobiologia (CAB), CSIC-INTA. Postal address: ESAC,
Camino Bajo del Castillo s/n,
28692,
Villanueva de la Cañada,
Madrid,
Spain
2
Jet Propulsion Laboratory, California Institute of Technology,
Pasadena,
CA
91109,
USA
★ Corresponding author; jalonso@cab.inta-csic.es
Key words: stars: AGB and post-AGB / binaries: close / circumstellar matter / stars: mass-loss / radio lines: stars / errata, addenda
This is a corrigendum to Alonso-Hernández et al. (2024). There was an error in the signs of the tabulated derived systemic velocities (Vsys) given in Table 3. That is, positive velocities are shown as negative and, equivalently, negative velocities are shown as positive. The analysis, results and conclusions of the paper are not affected by this error. The revised table is given below (Table 1).
References
- Alonso-Hernández, J., Sánchez Contreras, C., & Sahai, R. 2024, A&A, 684, A77 [NASA ADS] [CrossRef] [EDP Sciences] [Google Scholar]
© The Authors 2024
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