INSTABILITY ANALYSIS OF N=7; m=1 OSCILLATION HARMONICS FOR LOPSIDED STRUCTURES IN SELF-GRAVATING DISK-LIKE SYSTEMS

Аббас ОМОНОВ, Жахонгир ГАНИЕВ,, Фарход БОТИРОВ, Сабир ТУРАЕВ

Ўзбекистон Миллий университети хабарлари · 2024-yil

Annotatsiya

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.

Maqola ma’lumotlari
MualliflarАббас ОМОНОВ, Жахонгир ГАНИЕВ,, Фарход БОТИРОВ, Сабир ТУРАЕВ
JurnalЎзбекистон Миллий университети хабарлари
Nashr sanasi2024-03-29
Jild3
Son3.1
Betlar497-500
TilRus
DOI10.69617/nuuz.v3i3.1.1921

Kalit so‘zlar

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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