ANALYSIS OF THE EFFECT OF DISPLACEMENT OF THE CORE FROM THE GEOMETRIC CENTER OF SPIRAL GALAXIES

Abstract

To analyze the physics of the formation of galaxies and other gravitational systems, we first need to<br> create accurate analytically solvable models for them. Taking this into account, new analytical models<br> were created, and critical diagrams were found, forming analogs of nonlinear non-stationary<br> equations for the (1;3) mode, which corresponds to the displacement of the nucleus from the<br> geometric center, which occurs in spiral galaxies<br>

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DOI

10.5281/zenodo.7198968

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