|
|
Paper: |
Corrugated Velocity Pattern in NGC 5427 |
Volume: |
230, Galaxy Disks and Disk Galaxies |
Page: |
199 |
Authors: |
Alfaro, E. J.; Pérez, E.; González-Delgado, R.; Martos, M.; Franco, J. |
Abstract: |
Here we report the detection, in Hα emission, of a radial corrugation in the velocity field of the spiral galaxy NGC 5427. The central velocity of the Hα line displays coherent, wavy-like variations in the vicinity of the spiral arms. This kinematical behavior is similar to the one expected in a galactic bore generated by the interaction of a spiral wave with a thick gaseous disk, as recently modelled by Martos & Cox (1998). |
|
|
|
|