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

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

1995-02-15

arxiv.org/abs/astro-ph/9502073v2

Astronomy and Astrophysics

Astrophysics

Erroneous duplicate of astro-ph/9411031

Scientific paper

10.1086/175547

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

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