Gravitational instability of gas-dust circumnuclear disks in nearby galaxies
DOI:
https://doi.org/10.21638/spbu01.2022.316Abstract
Using the two-dimensional multi-component hydrodynamical simulations, we study the effect of dust on the development of instability in the gas-dust mini-disks observed in the central regions of galaxies. The dust is coupled with the gas gravitationally and by means of a friction force depending on the velocity difference between the two components. The presence of dust leads to the instability of a mini-disk and the development of a spiral structure observed in the gas-dust mini-disks. The spiral structure is multi-armed, which is caused by a dominance of the high order Fourier harmonics in the unstable modes. The instability of gas-dust circumnuclear disks is an important mechanism for explaining the activity of galactic nuclei associated with the accretion of matter onto a central black hole. We find that the admixture of dust with a dust-to-gas ratio of 10-20 % significantly destabilizes the gas-dust disk.Keywords:
circumnuclear disks, numerical simulations, computational hydrodynamics, galactic centres
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Articles of "Vestnik of Saint Petersburg University. Mathematics. Mechanics. Astronomy" are open access distributed under the terms of the License Agreement with Saint Petersburg State University, which permits to the authors unrestricted distribution and self-archiving free of charge.