Other
Scientific paper
Apr 1984
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984mnras.207..909i&link_type=abstract
Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 207, April 15, 1984, p. 909-927. Research supported by
Other
59
Astronomical Models, Galactic Evolution, Interstellar Gas, Molecular Clouds, Star Formation, Supernova Remnants, Gas Transport, Gravitational Collapse, Milky Way Galaxy, Phase Transformations, Secular Variations, Steady State
Scientific paper
The time variation of the interstellar medium regulated by supernova remnants is studied by considering the interchange processes among six components: a warm gas, a general ambient gas, a hot gas, small clouds, molecular clouds and giant molecular clouds. Two interesting results are found. One is that the interstellar medium does not always attain a steady state such as a two- or three-phase model, but may exhibit a cyclic phase-change like a limit cycle or go to a runaway state. The other is that bursts of star formation from molecular clouds are expected if the gravitational instability of a cloud ensemble is considered.
Habe Asao
Ikeuchi Satoru
Tanaka Y. D.
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