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The Hose-Pipe Instability in Stellar Systems

Published online by Cambridge University Press:  12 April 2016

R. M. Kulsrud ,
James W. K. Mark  and
A. Caruso
R. M. Kulsrud
Affiliation:
Plasma Physics Laboratory, Princeton University, Princeton, New Jersey 08540
James W. K. Mark
Affiliation:
Plasma Physics Laboratory, Princeton University, Princeton, New Jersey 08540
A. Caruso
Affiliation:
Laboratori Gas Ionizzati, Frascati, Italy

Extract

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Indications are that instabilities play an important role in many of the phenomena of stellar dynamics. Examples of such phenomena are: the formation of spiral arms, and the evolution of stellar clusters at a rate faster than one would expect from normal two-body collisions. The analogy with the situation in plasma physics, where similar phenomena are known to be dominated by instabilities, is very suggestive that one might seek for instabilities in stellar dynamics that correspond to similar ones in plasma physics.

Type
Research Article
Information
International Astronomical Union Colloquium , Volume 10: Gravitational N-Body Problem , November 1971 , pp. 52 - 55
Copyright
Copyright © Reidel 1971

References

Antonov, V. A.: 1960, Soviet Astron. 4, 859.Google Scholar
Antonov, V. A.: 1962, J. Leningrad Univ. 7, 135 (available in translation Princeton Plasma Physics Laboratory Report PPL-Trans-1 (1969) 34 pp.).Google Scholar
Ipser, J. R. and Thorne, K. S.: 1968, Astrophys. J. 154, 251.Google Scholar
Kulsrud, R. M. and Mark, J. W. K.: 1960, Astrophys. J. 160, 471.Google Scholar
Lynden Bell, D. and Sanitt, N.: 1969, Monthly Notices Roy. Astron. Soc. 143, 167.CrossRefGoogle Scholar
Milder, D. M.: 1969, ‘Rotating Stellar Systems’, unpubl. Ph.D. thesis, Harvard Univ.Google Scholar
Toomre, A.: 1966, ‘A Kelvin-Helmholtz Instability’, Notes from the Geophysical Fluid Dynamics Summer Program, Woods Hole Oceanographie Inst., pp. 111–114.Google Scholar