Can bar dynamics produce double-peaked profiles?
1 : Observatoire de Paris - Site de Paris
(OP)
-
Website
Observatoire de Paris, INSU, CNRS : UMR8112
61 Av de l'Observatoire 75014 PARIS -
France
2 : Collège de France
(CDF)
Collège de France
11 place Marcelin Berthelot F-75231 Paris Cedex 05 -
France
Star formation in barred galaxies is sometimes concentrated at the end of the bar, while the inner regions of the bar are quenched. I will review the possibility that at least some DP-galaxies could be due to this phenomenon.
| Subject : | : | oral |
| Topics | : | Morphology identification |
| PDF version | : |  PDF version |
