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Unstable spiral modes in disk-shaped galaxies: A general fluid dynamical theory with some preliminary results

A numerical scheme has been devised to calculate discrete spiral modes in a fluid-dynamical model of disk galaxies. The procedure is free from the usual restrictions imposed upon the asymptotic theory. A radiation condition has been formulated as one of the boundary conditions. For a test model gala...

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Bibliografiske detaljer
Main Authors: Pannatoni, R. F., Lau, Y. Y.
Format: Artigo
Sprog:Inglês
Udgivet: 1979
Fag:
Online adgang:https://ncbi.nlm.nih.gov/pmc/articles/PMC382863/
https://ncbi.nlm.nih.gov/pubmed/16592611
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