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Review of N-Body Models of Tidal Interactions

Published online by Cambridge University Press:  25 May 2016

L. T. Gardiner
L. T. Gardiner*
Affiliation:
Dept. of International Education, Sun Moon University, Rep. of Korea

Abstract

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Considerable progress has been made in the current decade with the help of N-body simulations towards a deeper understanding of the nature of the dynamical relationship between the Large and Small Magellanic Clouds and the Galaxy. The origin of such features as the Magellanic Stream, the inter-Cloud Bridge, the Wing and large extension in depth of the SMC has come to be interpreted in the context of the tidal interactions among the members of the LMC-SMC-Galaxy triple system. The inclusion of gas-dynamical effects and star formation in the latest models has added further refinements to this picture and confirmed the enhancement of the star formation rate in the SMC as a result of the recent LMC-SMC encounter.

Type
Part 7. Tidal Interactions
Information
Symposium - International Astronomical Union , Volume 190: New Views of the Magellanic Clouds , 1999 , pp. 480 - 486
Copyright
Copyright © Astronomical Society of the Pacific 1999 

References

Caldwell, J.A.R., & Coulson, I.M. 1986, MNRAS, 218, 223 Google Scholar
Gardiner, L.T. 1999, in “Proceedings from the Stromlo Workshop on High-Velocity Clouds”, eds Gibson, B.K., & Putman, M.E., p.292 Google Scholar
Gardiner, L.T., & Noguchi, M. 1996, MNRAS, 278, 191 (GN96) CrossRefGoogle Scholar
Gardiner, L.T., Sawa, T., & Fujimoto, M. 1994, MNRAS, 266, 567 Google Scholar
Grondin, L., Demers, S., & Kunkel, W.E. 1992, AJ, 103, 1234 Google Scholar
Hatzidimitriou, D., & Hawkins, M.R.S. 1989, MNRAS, 241, 667 Google Scholar
Irwin, M.J., Demers, S., & Kunkel, W.E. 1990, AJ, 99, 191 CrossRefGoogle Scholar
Kroupa, P., & Bastian, U. 1997, New Astron., 2, 77 Google Scholar
Kunkel, W.E., Demers, S., Irwin, M.J., & Albert, L. 1997, ApJ, 488, L129 Google Scholar
Lu, L., Savage, B.D., Sembach, K.R., Wakker, B.P., Sargent, W.L.W., & Oosterloo, T.A. 1998, AJ, 115, 162 Google Scholar
Moore, B., & Davis, M. 1994, MNRAS, 270, 209 Google Scholar
Murai, T., & Fujimoto, M. 1980, PASJ, 32, 581 Google Scholar
Noguchi, M. 1986, MNRAS, 219, 305 Google Scholar
Putman, M.E., Gibson, B.K., Staveley-Smith, L. et al., 1998, Nature, 394, 752 CrossRefGoogle Scholar
Yoshizawa, A. 1998, , Google Scholar