Instability of Stationary Spherical Models with Orbits Arbitrarily Close to Radial
The classical problem of the stability of stationary stellar spherical models with purely radial motion is reconsidered. The problem is due to strong central singularity in the density distribution, resulting in not entirely rigorous proof made in the well-known Antonov's paper. To avoid this d...
| Main Authors: | , |
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| Format: | Article |
| Language: | English |
| Published: |
De Gruyter
2016-12-01
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| Series: | Open Astronomy |
| Subjects: | |
| Online Access: | https://doi.org/10.1515/astro-2017-0254 |