The influence of inhomogeneity of the gaseous disk on the spiral structure parameters in galaxies with two-humped rotation curves

Details The influence of inhomogeneity of the gaseous disk on the spiral structure parameters in galaxies with two-humped rotation curves The influence of inhomogeneity of the gaseous disk on the spiral structure parameters in galaxies with two-humped rotation curves

Oct 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989kfnt....5...75m&link_type=abstract

Kinematika i Fizika Nebesnykh Tel (ISSN 0233-7665), vol. 5, Sept.-Oct. 1989, p. 75-80. In Russian.

Astronomy and Astrophysics

Astronomy

2

Galactic Structure, Gas Dynamics, Rotating Fluids, Spiral Galaxies, Astronomical Models, Flow Stability, Gas Density, Inhomogeneity, Thermodynamic Equilibrium

Scientific paper

The finite width 'jump' in the equilibrium surface density distribution
of the gaseous subsystem of a flat galaxy is studied. Emphasis is given
to the jump's influence on the parameters of spiral structure excited by
hydrodynamic instability. The results are compared with those of
numerical and analog experiments.

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