Evolution of dust disks and jets in dynamic equilibrium models. The role of “dark matter”

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A model of the structure and dynamics of dust disk structures under conditions of dynamic equilibrium is briefly presented. It is shown that an important role in the formation of the disk structure is played by the inhomogeneous distribution of the particle massiveness function in space, which is a model of “dark matter”. Disk structures that appear in the model may contain jets and bulges.

Dynamics of self-gravitating dust, dynamic equilibrium, structure of dust disks, jets, dark matter

Короткий адрес: https://sciup.org/142241068

IDR: 142241068   |   DOI: 10.17238/issn2226-8812.2024.1.54-58

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