The peculiar velocities of H I clouds

Details The peculiar velocities of H I clouds The peculiar velocities of H I clouds

Oct 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988pazh...14..902s&link_type=abstract

Pis'ma v Astronomicheskii Zhurnal (ISSN 0320-0108), vol. 14, Oct. 1988, p. 902-908. In Russian. In Russian.

Astronomy and Astrophysics

Astronomy

Flow Velocity, Gas Dynamics, H I Regions, Interstellar Gas, Rotating Fluids, Accretion Disks, Galactic Structure, Gas Heating, Supernovae

Scientific paper

A mechanism of "viscous heating" of gaseous systems along with the
commonly accepted mechanism of H I clouds peculiar velocity support by
supernovae explosions is shown to be operative in disk galaxies. This
mechanism is typical for differentially rotating systems.

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