Hostname: page-component-76fb5796d-9pm4c Total loading time: 0 Render date: 2024-04-27T01:27:18.514Z Has data issue: false hasContentIssue false
  • English
  • Français

Tumbling instability in oblate rotating stellar systems

Published online by Cambridge University Press:  07 August 2017

E. Szuszkiewicz ,
J.C.B. Papaloizou ,
A. J. Allen  and
P.L. Palmer
E. Szuszkiewicz
Affiliation:
School of Mathematical Sciences, Queen Mary & Westfield College, London
J.C.B. Papaloizou
Affiliation:
School of Mathematical Sciences, Queen Mary & Westfield College, London
A. J. Allen
Affiliation:
School of Mathematical Sciences, Queen Mary & Westfield College, London
P.L. Palmer
Affiliation:
School of Mathematical Sciences, Queen Mary & Westfield College, London

Abstract

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 present evolutionary calculations which show the tumbling instability found in spherical stellar systems by Allen et al. (1992) also occurs in some initially oblate rotating systems.

Type
Contributed Papers
Information
Symposium - International Astronomical Union , Volume 153: Galactic Bulges , 1993 , pp. 383 - 384
Copyright
Copyright © Kluwer 1993 

References

Allen, A.J., Palmer, P.L. & Papaloizou, J., 1990. Mon Not R astr Soc, 242, 576.CrossRefGoogle Scholar
Allen, A.J., Palmer, P.L. & Papaloizou, J., 1992. Mon Not R astr Soc, 256, 695.CrossRefGoogle Scholar
Kormendy, J., 1981. The Structure and Evolution of Normal Galaxies ed. Fall, S. M. & Lynden-Bell, D., Cambridge University Press.Google Scholar
Papaloizou, J., Palmer, P.L. & Allen, A.J., 1991. Mon Not R astr Soc, 253, 129.CrossRefGoogle Scholar