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Tidal Models of the Magellanic System

Published online by Cambridge University Press:  25 April 2016

R. A. Gingold
R. A. Gingold*
Affiliation:
Mount Stromlo and Siding Spring Observatories, Research School or Physical Sciences, The Australian National University
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Extract

Of the attempts to model the Magellanic system as the result of tidal interactions, only the works of Lin and Lynden-Bell (LLB 1982) and Murai and Fujimoto (MF 1981) can be considered to be successful.

Type
Contributions
Information
Publications of the Astronomical Society of Australia , Volume 5 , Issue 4 , 1984 , pp. 469 - 471
Copyright
Copyright © Astronomical Society of Australia 1984

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References

Lin, D. N. C., and Lynden-Bell, D., Mon. Not. K. Astron. Soc., 198, 707 (1982).Google Scholar
Mathewson, D. S., Proc. Astron. Soc. Aust., 3, 20 (1976).Google Scholar
Mathewson, D. S., Cleary, M. N., and Murray, J. D., Astrophys. J., 190, 291 (1974).CrossRefGoogle Scholar
Mathewson, D. S., and Ford, V. L., in The Structure and Evolution of the Magellanic Clouds, IAU #108, (Reidel) (1983).Google Scholar
Mathewson, D. S., and Schwarz, M. P., Mon. Not. R. Astron. Soc., 176, 47 (1976).Google Scholar
Mathewson, D. S., Schwarz, M. P., and Murray, J. D., Astrophys. J. (Letters), 217, L5 (1977).Google Scholar
Murai, T., and Fujimoto, M., Publ. Astron. Soc. Japan, 32, 581 (1980).Google Scholar
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Wood, P. R., Bessell, M. S., and Paltaglou, G., submitted to Astrophys. J. (1984).Google Scholar