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Companion Driven Spirals and Bars

Published online by Cambridge University Press:  03 August 2017

E. Athanassoula
E. Athanassoula*
Affiliation:
Observatoire de Marseille 2, Place Le Verrier F-13248 MARSEILLE Cedex 04 FRANCE

Extract

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With the help of a series of N-body simulations made with J. Sellwood's code I have studied the properties of spirals and bars in interacting galaxies. I will give here only a brief summary of the main results. For more information see Athanassoula (1990 and in prep.)

Type
VIII- Bars, Rings and Starbursts
Information
Symposium - International Astronomical Union , Volume 146: Dynamics of Galaxies and their Molecular Cloud Distributions , 1991 , pp. 274 - 276
Copyright
Copyright © Kluwer 1991 

References

References :

1. Athanassoula, E.: 1990, in “Chemical and Dynamical Evolution of Galaxies”, Eds. Franco, J. and Matteuci, F. (World Scientific), in press.Google Scholar
2. Gerin, M., Combes, F. and Athanassoula, E.: 1990, Astr. and Astrophys. 230, 37.Google Scholar
3. Noguchi, M. 1987: Mon. Not. Roy. Astr. Soc. 228, 535.Google Scholar