The occurrence of lopsided structures in self-gravitating disk-like systems was studied by means of a pulsating non-stationary disk-like model. Azimuthal wave number m=1, radial wave number N=7 for oscillation harmonics, creating an analogue of non-stationary dispersion equations (NADR) and through their numerical solutions, critical diagrams were obtained and the type of instability was determined.
| Mualliflar | Аббас ОМОНОВ, Жахонгир ГАНИЕВ,, Фарход БОТИРОВ, Сабир ТУРАЕВ |
|---|---|
| Jurnal | Ўзбекистон Миллий университети хабарлари |
| Nashr sanasi | 2024-03-29 |
| Jild | 3 |
| Son | 3.1 |
| Betlar | 497-500 |
| Til | Rus |
| DOI | 10.69617/nuuz.v3i3.1.1921 |
DOI: 10.69617/nuuz.v3i3.1.1921 · Maqolaning asl sahifasi
galaxy: -lopsided, accretion, evolution, matter, model: -superposition, critical, isotropic, pulsation, amplitude, rotation., галактики: - лопсаидальной, аккреция, эволюция, материя, модель: - суперпозиция, критическая, изотропная, пульсация, амплитуда, вращение., galaktika:- lopsaidal, akkretsiya, evolyutsiya, materiya, model:-superpozitsiya, kritik, izotrop, pulsatsiya, amplituda, aylanish.
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