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Periodic Orbits and Warps

Published online by Cambridge University Press:  04 August 2017

W. A. Mulder*
Affiliation:
Sterrewacht, Huygens Laboratorium, P.O. Box 9513, 2300 RA Leiden, The Netherlands

Extract

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Orbit calculations were done in a rotating triaxial system with a density distribution in accordance with recent observations of spiral galaxies. A search was made for simple closed orbits which are tilted with respect to the plane of the galaxy. A family of stable prograde tilted orbits was found which can explain warps as stationary phenomena.

Type
III. Warps
Copyright
Copyright © Reidel 1983 

References

Bertola, R., Galleta, G.: 1978, Astrophys. J. 226, L115.CrossRefGoogle Scholar
Binney, J.: 1981, Monthly Notices Roy. Astron. Soc. 196, 455.CrossRefGoogle Scholar
Burstein, D., Rubin, V.C., Thonnard, N., Ford, W.K.: 1982, Astrophys. J. 253, 70.Google Scholar
Hawarden, T.G., Elson, R.A.W., Longmore, A.J., Tritton, S.B., Corwin, H.G.: 1981, Monthly Notices Roy. Astron. Soc. 196, 747.Google Scholar
Heisler, J., Merritt, D., Schwarzschild, M.: 1982, Astrophys. J. 258, 490.Google Scholar
Isaacman, R.B.: 1981, Astron. Astrophys. 95, 46.Google Scholar
Magnenat, P.: 1982, Astron. Astrophys. 108, 84.Google Scholar
Sanders, R.H., Lowinger, T.: 1972, Astrophys. J. 77, 242.Google Scholar