Formation of large-scale structure of the interstellar medium by interaction between clouds

Astronomy and Astrophysics – Astrophysics

Scientific paper

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Galactic Structure, Interstellar Matter, Molecular Clouds, Spiral Galaxies, Astronomical Models, Galactic Evolution, Galactic Rotation, Gravitational Effects, Viscosity

Scientific paper

The paper presents the results of calculations of the evolution of the density distribution of a 'gas of clouds' under the influence of viscosity. Due to this viscosity effect, ring-shaped formations consisting of clouds must develop in spiral galaxies. It is suggested that the occurrence of massive molecular complexes in the ring-shaped structures may be attributed to the gravitational instability of the 'gas of clouds'.

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