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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 

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