Hostname: page-component-77c89778f8-cnmwb Total loading time: 0 Render date: 2024-07-16T13:28:09.462Z Has data issue: false hasContentIssue false
  • English
  • Français

Hydrodynamical Models of Offcentered Barred Spirals

Published online by Cambridge University Press:  04 August 2017

J. Colin  and
E. Athanassoula
J. Colin
Affiliation:
Observatoire de Besançon ERA 07904 25000 Besançon - France
E. Athanassoula
Affiliation:
Observatoire de Besançon ERA 07904 25000 Besançon - France

Extract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

We have studied the flow of gas in barred spirals in which the centers of the bar and the disk do not coincide. This is often observed in late type galaxies like the L.M.C., NGC 1313, NGC 4618 etc…

Type
IV. Barred Galaxies
Information
Symposium - International Astronomical Union , Volume 100: Internal Kinematics and Dynamics of Galaxies , 1983 , pp. 239 - 240
Copyright
Copyright © Reidel 1983 

References

Sanders, R.H., Tubbs, A.D. : 1980, Astrophys. J., 235, 803.CrossRefGoogle Scholar