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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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Hlavní autoři: Lau, Y. Y., Mark, James W.-K.
Médium: Artigo
Jazyk:Inglês
Vydáno: 1976
Témata:
On-line přístup:https://ncbi.nlm.nih.gov/pmc/articles/PMC431208/
https://ncbi.nlm.nih.gov/pubmed/16592357
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