Issue |
A&A
Volume 564, April 2014
|
|
---|---|---|
Article Number | C1 | |
Number of page(s) | 1 | |
Section | Extragalactic astronomy | |
DOI | https://doi.org/10.1051/0004-6361/201322288e | |
Published online | 17 April 2014 |
ALMA observations of feeding and feedback in nearby Seyfert galaxies: an AGN-driven outflow in NGC 1433 (Corrigendum)⋆
1
Observatoire de Paris, LERMA, CNRS: UMR 8112, 61 Av. de
l’Observatoire,
75014
Paris,
France
e-mail:
francoise.combes@obspm.fr
2
Observatorio Astronómico Nacional (OAN)-Observatorio de
Madrid, Alfonso XII,
3, 28014
Madrid,
Spain
3
INAF – Istituto di Radioastronomia & Italian ALMA Regional
Centre, via Gobetti 101, 40129
Bologna,
Italy
4
INAF – Osservatorio Astrofisico di Arcetri, Largo E. Fermi
5, 50125
Firenze,
Italy
5
IRAM, 300 rue de la Piscine, Domaine Universitaire,
38406 Saint Martin
d’Hères,
France
6
Dep. of Physics & Astronomy, Rutgers, the State University
of New Jersey, 136 Frelinghuysen
road, Piscataway,
NJ
08854,
USA
7
CNRS, IRAP, 9
Av. colonel Roche, BP
44346, 31028
Toulouse Cedex 4,
France
8
I. Physikalisches Institut, Universität zu Köln,
Zülpicher Str. 77, 50937
Köln,
Germany
9
Instituto de Astrofisica de Andalucía (CSIC),
Apdo 3004, 18080
Granada,
Spain
10
Max-Planck-Institut für Astronomie (MPIA),
Königstuhl 17, 69117
Heidelberg,
Germany
11
Max-Planck-Institut für extraterrestrische Physik,
Giessenbachstr. 1, Garching bei
München, 81679
München,
Germany
Key words: galaxies: active / galaxies: individual: NGC 1433 / galaxies: ISM / galaxies: kinematics and dynamics / galaxies: nuclei / errata, addenda
In Sect. 4. Discussion and summary, an error has occurred in the estimation of the momentum flux of the outflow in NGC 1433. The momentum flux was estimated to be larger than that provided by the AGN photons LAGN/c by a factor 2000 tanα/cosα, while it is in reality larger by only a factor 10 tanα/cosα. With the new value, AGN radio jets are not required, and an energy-conserving AGN wind would be sufficient to account for the outflow.
© ESO, 2014
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