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Polygonal Structures in a Gaseous Disk: Numerical Simulations

Наименование публикации Polygonal Structures in a Gaseous Disk: Numerical Simulations
Тип публикации Статья
Библиографическое описание Polygonal Structures in a Gaseous Disk: Numerical Simulations / S. A. Khoperskov, A. V. Khoperskov, M. A. Eremin, M. A. Butenko // Astronomy Letters. — 2011. — Vol. 37, No. 8. — Pp. 563-575.
Аннотация The results of numerical simulations of a gaseous disk in the potential of a stellar spiral density wave are presented. The conditions under which straightened spiral arm segments (rows) form in the gas component are studied. These features of the spiral structure were identified in a series of works by A.D. Chernin with coauthors. Gas-dynamic simulations have been performed for a wide range of model parameters: the pitch angle of the spiral pattern, the amplitude of the stellar spiral density wave, the disk rotation speed, and the temperature of the gas component. The results of 2D- and 3D-disk simulations are compared. The rows in the numerical simulations are shown to be an essentially nonstationary phenomenon. A statistical analysis of the distribution of geometric parameters for spiral patterns with rows in the observed galaxies and the constructed hydrodynamic models shows good agreement. In particular, the numerical simulations and observations of galaxies give α~120◦ for the average angles between straight segments.
Ключевые cлова numerical gas dynamics, shock waves, spiral structure of galaxies
Год публикации 2011
Хоперсков Сергей Александрович
Электронная копия публикации Загрузить