Unstable spiral modes in disk-shaped galaxies: Enhancement of growth rate
An additional effect not considered in our earlier papers is found to enhance the rate of growth of spiral modes in disk-shaped galaxies. This enhanced growth appears to be attributable to the combined influence of differential rotation and tangential forces. For certain galaxy models, rapid tempora...
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| Publicado en: | Proc Natl Acad Sci U S A |
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| Autores principales: | , |
| Formato: | Artigo |
| Lenguaje: | Inglês |
| Publicado: |
National Academy of Sciences
1976
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| Materias: | |
| Acceso en línea: | https://ncbi.nlm.nih.govhttps://pmc.ncbi.nlm.nih.gov/articles/PMC431208/ https://ncbi.nlm.nih.govhttps://pubmed.ncbi.nlm.nih.gov/16592357/ https://ncbi.nlm.nih.govhttps://doi.org/10.1073/pnas.73.11.3785 |
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