A new criterion for Bar-Forming Instability in Rapidly Rotating Gaseous and Stellar Systems. I. Axisymmetric Form
arXiv:astro-ph/9502073 · doi:10.1086/175547
Abstract
This paper has been removed by arXiv admin because it was an erroneous duplicate of astro-ph/9411031.
Erroneous duplicate of astro-ph/9411031