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Dynamical Behaviour of Gaseous Halo in a Disk Galaxy

Published online by Cambridge University Press:  14 August 2015

S. Ikeuchi  and
A. Habe
S. Ikeuchi
Affiliation:
Department of Physics, Hokkaido University, Sapporo 060, Japan
A. Habe
Affiliation:
Department of Physics, Hokkaido University, Sapporo 060, Japan

Extract

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Assuming that the gas in the halo of a disk galaxy is supplied from the disk as a hot gas, we have studied its dynamical and thermal behaviour by means of a time dependent, two-dimensional hydrodynamic code.

Type
Research Article
Information
Symposium - International Astronomical Union , Volume 94: Origin of Cosmic Rays , 1981 , pp. 275 - 276
Copyright
Copyright © Reidel 1981 

References

Bregman, J. N.: 1979, Ap. J., 229, 514.Google Scholar
Bregman, J. N.: 1980, Ap. J., 236, 577.Google Scholar
McKee, C. F., and Ostriker, J. P.: 1977, Ap. J., 211, 148.Google Scholar