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Large-scale Gas Dynamical Processes Affecting the Origin and Evolution of Gaseous Galactic Halos
1991
Symposium - International astronomical union
Observations of galactic halo gas are consistent with an interpretation in terms of the galactic fountain model in which supernova heated gas in the galactic disk escapes into the halo, radiatively cools and forms clouds which fall back to the disk. The results of a new study of several large-scale gas dynamical effects which are expected to occur in such a model for the origin and evolution of galactic halo gas will be summarized, including the following: (1) nonequilibrium absorption line and
doi:10.1017/s0074180900089373
fatcat:yv5baoheanfuxhfyt3ibraztga