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Particle resonance in a spiral field

Published online by Cambridge University Press:  14 August 2015

B. Barbanis
B. Barbanis*
Affiliation:
Dept. of Astronomy, University of Patras, Greece

Abstract

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Plane galactic orbits near the particle resonance of a spiral field have been calculated numerically. Besides the ring type orbits, i.e. orbits filling a ring around the galactic center, there are orbits librating near the potential maxima at the co-rotation distance (Lagrangian points). This effect tends to disrupt the spiral arms at the co-rotation distance.

Type
Part III/Theory of Spiral Structure
Information
Symposium - International Astronomical Union , Volume 38: The Spiral Structure of our Galaxy , 1970 , pp. 343 - 347
Copyright
Copyright © Reidel 1970 

References

Barbanis, B.: 1968a, Astrophys. J. 153, 71.Google Scholar
Barbanis, B.: 1968b, Astron. J. 73, 784.CrossRefGoogle Scholar
Barbanis, B. and Woltjer, L.: 1967, Astrophys. J. 150, 461.CrossRefGoogle Scholar
Contopoulos, G. and Strömgren, B.: 1965, Tables of Plane Galactic Orbits, Inst. Space Studies, New York.Google Scholar
Lin, C. C., Yuan, C., and Shu, F.: 1969, Astrophys. J. 155, 721.CrossRefGoogle Scholar
Marochnik, L. S. and Suchkov, A. A.: 1969, Astrophys. Space Sci. 4, 317.Google Scholar