Condensation of small spherical non-gravitationally bound cool clouds

Details Condensation of small spherical non-gravitationally bound cool clouds Condensation of small spherical non-gravitationally bound cool clouds

Jan 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987a%26a...172..280p&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 172, no. 1-2, Jan. 1987, p. 280-292. Research supported by the Universidad de

Astronomy and Astrophysics

Astrophysics

24

Condensing, Interstellar Chemistry, Interstellar Gas, Molecular Clouds, Thermal Instability, Astronomical Models, Galactic Evolution, Gravitational Fields, Milky Way Galaxy, Supernova Remnants, Supernovae

Scientific paper

A model for the interstellar medium (ISM) is discussed, including the mechanisms of ionization, recombination, cooling and heating. The formation and subsequeent evolution of spherical, nonmagnetic small clouds due to thermochemical instabilities in the interstellar warm gas are considered. Appreciable differences in the thermoionic structure appear when the ionization inertia is taken into account. Numerical solutions for the thermochemical structure and for the rate of condensation are obtained. It is shown that small clouds play an important role in the ISM balance.

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