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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| Publicat a: | Proc Natl Acad Sci U S A |
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| Autors principals: | , |
| Format: | Artigo |
| Idioma: | Inglês |
| Publicat: |
National Academy of Sciences
1979
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| Matèries: | |
| Accés en línia: | https://ncbi.nlm.nih.govhttps://pmc.ncbi.nlm.nih.gov/articles/PMC382863/ https://ncbi.nlm.nih.govhttps://pubmed.ncbi.nlm.nih.gov/16592611/ https://ncbi.nlm.nih.govhttps://doi.org/10.1073/pnas.76.1.4 |
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