Simulation of the spiral structure of galaxies in a rotating liquid

Details Simulation of the spiral structure of galaxies in a rotating liquid Simulation of the spiral structure of galaxies in a rotating liquid

Jun 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984zhpmr..39..504m&link_type=abstract

(ZHETF Pis'ma v Redaktsiiu, vol. 39, June 10, 1984, p. 504-507) JETP Letters (ISSN 0021-3640), vol. 39, June 10, 1984, p. 613-61

Physics

7

Density Wave Model, Galactic Structure, Rotating Fluids, Spiral Galaxies, Hydrodynamics, Simulation, Velocity Distribution, Water Flow

Scientific paper

The hydrodynamic theory of the formation of the spiral structure of galaxies with a rapidly rotating core is confirmed by an experiment in rotating shallow water. There is an analogous ('supersonic') discontinuity in the velocity profile of the water. The water exhibits a theoretically predicted new centrifugal instability, which generates a spiral pattern.

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