A numerical model of a triple system with hidden masses

Mathematics – Dynamical Systems

Scientific paper

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Astronomical Models, Dark Matter, Gravitational Effects, Ternary Systems, Coalescing, Collision Parameters, Dynamical Systems, Isothermal Processes, Stellar Rotation

Scientific paper

The paper presents a numerical model of a triple system of gravitating bodies with hidden matter distributed continuously according to the isothermal law. It is shown that the presence of hidden mass prevents contact collisions and the coalescence of the system components. The issue of the predominance of weakly rotating stellar systems (E-galaxy type) in groups with large hidden masses is addressed.

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