On the radial distributions of molecular clouds in galaxies

Details On the radial distributions of molecular clouds in galaxies On the radial distributions of molecular clouds in galaxies

Feb 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986ap%26ss.119..143f&link_type=abstract

(IAU, Asian-Pacific Regional Meeting, 3rd, Kyoto, Japan, Sept. 30-Oct. 5, 1984) Astrophysics and Space Science (ISSN 0004-640X),

Astronomy and Astrophysics

Astrophysics

3

Galactic Structure, Interstellar Gas, Molecular Clouds, Radial Distribution, Gas Dynamics, Radial Flow, Viscosity

Scientific paper

The dynamics of the interstellar gas (the IS gas) driven by the viscous
torque of a system of giant molecular clouds (the MC gas) is considered
with the infinitesimally thin disk layer approximation. The flow
explains the radial distributions of molecules observed in galaxies.

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