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Galactic Slow Bar as an Unstable Mode of a Stellar Disk
Published online by Cambridge University Press: 12 April 2016
Abstract
An estimate for the slow bar instability boundary for a generalized disk polytropic model is derived. The effects of a spherical halo are studied: it turns out that a halo can be favorable to this instability (at the same time suppressing the bending instability).
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- Posters of Part VII and Part VIII
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- Copyright © Astronomical Society of the Pacific 1996