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ON THE THEORY OF THE ORIGIN OF THE BULGE OF SPIRAL GALAXIES. 1. DOME PERTURBATION MODE

Botirov Farkhod UktamovichNational University of Uzbekistan
ABI

Abstract

To develop an origin theory of galactic bulges the gravitational instabilities of oscillation modes (0,3) and (2,2) have been studied on the background of two non-linearly non-stationary models: anisotropic disk-like system and Kamm’s model.

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