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Box Models without Cylindrical Rotation

Published online by Cambridge University Press:  04 August 2017

Maria Petrou
Maria Petrou*
Affiliation:
Department of Theoretical Physics, 1 Keble Road, Oxford, OX1 3NP, United Kingdom

Abstract

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We describe here a way of constructing models for box–shaped dynamical systems without cylindrical rotation. We argue that such models may arise as a result of the external heating of a disk.

Type
Posters
Information
Symposium - International Astronomical Union , Volume 127: Structure and Dynamics of Elliptical Galaxies , 1987 , pp. 501 - 502
Copyright
Copyright © Reidel 1987 

References

4. REFERENCES

Binney, J.J. and Petrou, M., 1985, Mon. Not R. astr. Soc., 214, 449 Google Scholar
Hénon, M., 1960, Ann. d'Astrophys, 23, 474 Google Scholar