Hydrodynamic vortices in the gaseous disks of galaxies

Physics

Scientific paper

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Galaxies, Gas Dynamics, Interstellar Gas, Vortices, Flow Velocity, Hydrodynamic Equations, Solitary Waves, Steady Flow, Two Dimensional Flow

Scientific paper

A two-dimensional gas stream with a velocity field vx proportional to y is considered which is assumed to be stationary with respect to a rotating coordinate system. This stream can serve as a model of the local kinematic of a galactic gaseous disk. It is shown the local uniform stream cannot develop into a soliton if self-gravitation, dissipation, and the nonuniformity of the vortex are neglected.

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