The issues of instability of individual oscillation modes for a nonlinear nonstationary model of collapsing galaxy clusters have been studied. The instability of the model with respect to two disturbance modes is investigated. For each mode, the critical dependence of the initial virial ratio on the rotation parameter is constructed. The dependences of the instability increments on the physical parameters of the model are found.
| Mualliflar | Кутлимуратов, С., Отожанова, Н., И. Таджибаев, И. |
|---|---|
| Jurnal | O‘zbekiston fizika jurnali |
| Nashr sanasi | 2024-10-13 |
| Jild | 26 |
| Son | 3 |
| Til | Rus |
| DOI | 10.52304/.v26i3.533 |
DOI: 10.52304/.v26i3.533 · Maqolaning asl sahifasi
галактика, скопления, модель, вселенная, самогравитирующих систем, galaxy, clusters, model, universe, self-gravitating systems
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