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The Origin of Inner Rings in Barred Spiral Galaxies

Published online by Cambridge University Press:  25 April 2016

M. P. Schwarz
M. P. Schwarz*
Affiliation:
Mathematics Department, Monash University
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Extract

A large number of barred spiral galaxies contain a ring-like structure surrounding the bar. This is known as an inner ring if the bar terminates at the ring. Structures which are not closed but which appear to be related phenomena are given the name pseudo-inner rings by de Vaucouleurs (1959).

Type
Contributions
Information
Publications of the Astronomical Society of Australia , Volume 5 , Issue 4 , 1984 , pp. 464 - 467
Copyright
Copyright © Astronomical Society of Australia 1984

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References

Buta, R., Ph.D. Thesis, University of Texas (1984).Google Scholar
de Vaucouleurs, G., Handbuch der Physik, 53, 275 (1959).Google Scholar
Schwarz, M. P., Ph.D. Thesis, Australian National University (1979).Google Scholar
Schwarz, M. P., Astron. Astrophys., 133, 22 (1984a).Google Scholar
Schwarz, M. P., Mon. Not. R. Astron. Soc., in press, p. 208 (1984b).Google Scholar
Sellwood, J., Astron. Astrophys., 99, 363 (1981).Google Scholar