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Astron. Astrophys. 344, 719 (1999)

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A kinematical analysis of NGC 2992

I. Márquez 1,2, C. Boisson 3, F. Durret 2,3 and P. Petitjean 2,3

1 Instituto de Astrofísica de Andalucía (C.S.I.C.), Apartado 3004, E-18080 Granada, Spain
2 Institut d'Astrophysique de Paris, CNRS, Université Pierre et Marie Curie, 98 bis Bd Arago, F-75014 Paris, France
3 DAEC, Observatoire de Paris, Université Paris VII, CNRS (UA 173), F-92195 Meudon Cedex, France

Astron. Astrophys. 333, 459-465 (1998)

The outflow included in the model is indeed perpendicular to the galaxy plane, not parallel, as mentioned in the text.

We thank Mark G. Allen for pointing out this mistake.

Send offprint requests to: I. Márquez, IAA, Spain

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© European Southern Observatory (ESO) 1999

Online publication: March 18, 1999