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
astro-pharXiv:astro-ph/9502073
Abstract
This paper has been removed by arXiv admin because it was an erroneous duplicate of astro-ph/9411031.
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