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Instabilities in a nonstationary model of self-gravitating disks. III. The phenomenon of lopsidedness and a comparison of perturbation modes

K. T. MirtadjievaAstronomical Institute, Academy of Sciences of the Republic of Uzbekistan, Tashkent, UzbekistanС. Н. НуритдиновDepartment of Astronomy and Astrophysics, National University of Uzbekistan, Tashkent, UzbekistanJ. K. RuzibaevAstronomical Institute, Academy of Sciences of the Republic of Uzbekistan, Tashkent, UzbekistanMuhammad Khalid
Astrophysicsjournal2011en
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