Modeling stellar-gaseous disks: rows in spiral patterns of galaxies

The work is aimed at studying the formation mechanisms of straightened segments (rows) in spiral galactic arms, which are found in approximately 5% of S-galaxies. We use the Smoothed Particles Hydrodynamics (SPH) numerical algorithm, which is adapted for parallel computing on the GPUs to simulate th...

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Veröffentlicht in:	Journal of physics. Conference series 2019-04, Vol.1203 (1), p.12062
Hauptverfasser:	Butenko, Maria, Khoperskov, Alexander, Khrapov, Sergey
Format:	Artikel
Sprache:	eng
Schlagworte:	Algorithms Astronomical models Computational fluid dynamics Fluid flow Galaxies Hydrodynamics Numerical analysis Numerical models
Online-Zugang:	Volltext
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