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Gas dynamics and disk-galaxy evolution

Published online by Cambridge University Press:  04 August 2017

R. G. Carlberg*
Affiliation:
University of Toronto

Extract

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Gas dynamics plays a vital role in the formation and ongoing evolution of a disk galaxy through its ability to have dissipative collisions. In this paper the simplest possible gas physics which provides a description of a gaseous component is incorporated into N-body experiments to investigate the formation of a disk galaxy.

Type
PART III: Dynamics and Evolution
Copyright
Copyright © Reidel 1985 

References

Bregman, J.N. 1980, Ap. J., 236, p. 557.Google Scholar
Fall, S.M. and Efstathiou, G. 1980, M.N.R.A.S., 193, p. 189.Google Scholar
Larson, R.B. 1976, M.N.R.A.S., 176, p. 31.Google Scholar
McKee, C.F. and Ostriker, J.P. 1977, Ap. J., 218, p. 148.Google Scholar
Searle, L. and Zinn, R. 1978, Ap. J., 225, p. 357.CrossRefGoogle Scholar
White, S.D.M. and Rees, M.J. 1978, M.N.R.A.S., 183, p. 341.Google Scholar
Zinn, R. 1980, Ap. J., 241, p. 602.Google Scholar