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This article is cited in 3 scientific papers (total in 3 papers)
Physics and astronomy
Numerical simulation of the galaxies outer spiral structure: the influence of the dark halo non-axisymmetry on the gaseous disk shape
M. A. Butenko, I. V. Belikova, N. M. Kuz'min, S. S. Khokhlova, G. S. Ivanchenko, A. V. Tån, I. G. Kudina Volgograd State University
Abstract:
A detailed analysis of the results of numerical simulation of the outer spiral structure in a gaseous galactic disk caused by the presence of non-axisymmetry in the distribution of matter in a dark halo have been fulfilled. The result obtained in our previous work [8] that the non-axisymmetry of the gaseous disk is less than the non-axisymmetry in the dark mass distribution for disks with a spiral structure extending far beyond the optical radius, have been confirmed. Also, the result has been generalized for the dark halo model, which is spherical within the optical radius and non-axisymmetric beyond it.
Keywords:
hydrodynamics, outer spiral structure, numerical simulation, dark halo, non-axisymmetry.
Received: 25.07.2021 Accepted: 09.09.2022
Citation:
M. A. Butenko, I. V. Belikova, N. M. Kuz'min, S. S. Khokhlova, G. S. Ivanchenko, A. V. Tån, I. G. Kudina, “Numerical simulation of the galaxies outer spiral structure: the influence of the dark halo non-axisymmetry on the gaseous disk shape”, Mathematical Physics and Computer Simulation, 25:3 (2022), 73–83
Linking options:
https://www.mathnet.ru/eng/vvgum336 https://www.mathnet.ru/eng/vvgum/v25/i3/p73
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Abstract page: | 85 | Full-text PDF : | 32 |
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