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N-Body Simulations of the Magellanic System Including Gas Dynamics and Star Formation

Published online by Cambridge University Press:  25 May 2016

A.M. Yoshizawa  and
M. Noguchi
A.M. Yoshizawa
Affiliation:
Astronomical Institute, Tohoku University, Aoba, Sendai 980-77, Japan
M. Noguchi
Affiliation:
Astronomical Institute, Tohoku University, Aoba, Sendai 980-77, Japan

Extract

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The system of the Magellanic Clouds is considered to be dynamically interacting among themselves and with our Galaxy. This interaction is thought to be the cause of many complicated features seen in the Magellanic Clouds and the Magellanic Stream (see Westerlund 1990, A&AR, 2, 27). In order to better understand the formation and evolution of the Magellanic System, we carry out realistic N-body simulations of the tidal distortion of the Small Magellanic Cloud (SMC) due to our Galaxy and the Large Magellanic Cloud (LMC).

Type
Local Group
Information
Symposium - International Astronomical Union , Volume 186: Galaxy Interactions at High and Low Redshift , 1999 , pp. 60
Copyright
Copyright © Kluwer 1999