The effect of turbulence on radial motion in the gaseous disks of galaxies

Details The effect of turbulence on radial motion in the gaseous disks of galaxies The effect of turbulence on radial motion in the gaseous disks of galaxies

Feb 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990kfnt....6...73k&link_type=abstract

Kinematika i Fizika Nebesnykh Tel (ISSN 0233-7665), vol. 6, Jan.-Feb. 1990, p. 73-78. In Russian.

Computer Science

Sound

1

Galactic Rotation, High Temperature Gases, Radial Flow, Rotating Fluids, Turbulence Effects, Gas Dynamics, Hydrodynamic Equations

Scientific paper

A hydrodynamical model of gas rotation in galaxy disks is examined. It is shown that stationary rotation of a hot gas must be accompanied by intense turbulence and the accretion of matter onto the center of the galaxy. It is found that the intensity of turbulence, the velocities of ordered and turbulent radial motion, and accretion rates are all dependent on sound velocity.

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