Formation of Triaxial Galaxy

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Results of N-body simulation of dissipationless cold collapse of spherical gravitating system are presented. We compared the results with properties of elliptical galaxies. The system gradually evolved to triaxial system. The projected density profile is in good agreement with observations. In addition to triaxial instability, it seems that there is another instability
Publisher
THE KOREAN SPACE SCIENCE SOCIETY
Issue Date
1987-06
Language
Korean
Citation

JOURNAL OF ASTRONOMY AND SPACE SCIENCE, v.4, no.1, pp.1 - 10

URI
http://hdl.handle.net/10203/61724
Appears in Collection
PH-Journal Papers(저널논문)
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