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Studies on the Galactic Density Wave

Published online by Cambridge University Press:  07 February 2017

James W.-K. Mark
James W.-K. Mark*
Affiliation:
Massachusetts Institute of Technology, Cambridge, Mass., U.S.A.

Abstract

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For spiral galaxies, investigations have been made as to the behaviour of density waves at the critical regions of the Lindblad and co-rotation resonances and in particular as to their role in the maintenance and generation of these waves. We shall also discuss the conditions under which an inner resonance ring may be formed. Furthermore, we find that the co-rotation region acts as a wave-amplifier.

Type
Research Article
Information
Symposium - International Astronomical Union , Volume 58: The Formation and Dynamics of Galaxies , 1974 , pp. 417 - 423
Copyright
Copyright © Reidel 1974 

References

Contopoulos, G.: 1970, Astrophys. J. 160, 113.CrossRefGoogle Scholar
Lin, C. C.: 1969, in Becker, W. and Contopoulos, G. (eds), ‘The Spiral Structure of Our Galaxy’, IAU Symp. 38, 377.Google Scholar
Lin, C. C. and Feldman, S.: 1970, Ref. Lin, C. C., Highlights of Astron. 2, 88, 1971.Google Scholar
Lin, C. C., Yuan, C., and Shu, F. H.: 1969, Astrophys. J. 155, 721.CrossRefGoogle Scholar
Lynden-Bell, D. and Kalnajs, A.: 1972, Monthly Notices Roy. Astron. Soc. 157, 1.Google Scholar
Mark, J. W-K.: 1971, Proc. Nat. Acad. Sci. 68, 2095.Google Scholar
Mezger, P. G.: 1969, in Becker, W. and Contopoulos, G. (eds), ‘The Spiral Structure of Our Galaxy’, IAU Symp. 38, 107.Google Scholar
Toomre, A.: 1969, Astrophys. J. 158, 899.Google Scholar
van Woerden, H.: 1965, Ref. Oort, J. H., Trans. IAU 12A, 789.Google Scholar