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A new criterion for Bar-Forming Instability in Rapidly Rotating Gaseous and Stellar Systems. I. Axisymmetric Form

D. M. Christodoulou·I. Shlosman·J. E. Tohline
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This paper has been removed by arXiv admin because it was an erroneous duplicate of astro-ph/9411031.

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D. M. Christodoulou, I. Shlosman, J. E. Tohline. 2007-10-16. A new criterion for Bar-Forming Instability in Rapidly Rotating Gaseous and Stellar Systems. I. Axisymmetric Form. https://doi.org/10.1086/175547

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