INSTABILITY ANALYSIS OF N=7; m=1 OSCILLATION HARMONICS FOR LOPSIDED STRUCTURES IN SELF-GRAVATING DISK-LIKE SYSTEMS
Keywords:
galaxy: -lopsided, accretion, evolution, matter, model: -superposition, critical, isotropic, pulsation, amplitude, rotation.
Abstract
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.
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2. Chanda J. Jog et al//Physics Reports-2009
3. Rix H.-W., Zaritsky D., 1995, ApJ, 447, 82
4. Jog et al: AP.J-1997; MNRAS-2006; Phys,rev-2009
5. Beale, J.S., & Davies, R.D. 1969, Nature, 221, 531
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Published
2024-03-29
How to Cite
Аббас ОМОНОВ, Жахонгир ГАНИЕВ, Фарход БОТИРОВ, & Сабир ТУРАЕВ. (2024). INSTABILITY ANALYSIS OF N=7; m=1 OSCILLATION HARMONICS FOR LOPSIDED STRUCTURES IN SELF-GRAVATING DISK-LIKE SYSTEMS. News of the NUUz, 3(3.1), 497-500. https://doi.org/10.69617/uzmu.v3i3.1.1921
Section
Articles