A kinematical analysis of NGC 2992
I. Márquez 1,2,
C. Boisson 3,
F. Durret 2,3 and
P. Petitjean 2,3
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
© European Southern Observatory (ESO) 1999
Online publication: March 18, 1999