A MODEL FOR ELLIPTICAL RADIO GALAXIES WITH DUST LANES

被引：209
作者：
VANALBADA, TS
KOTANYI, CG
SCHWARZSCHILD, M
机构：
[1] Kapteyn Astronomical Institute, Postbus 800, Groningen,9700 AV, Netherlands
来源：
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | 1982年 / 198卷 / 01期
关键词：
Galaxies;
D O I：
10.1093/mnras/198.2.303
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
We describe the stationary states of motion of gas in a triaxial stellar system which rotates about one of its principal axes. Four dynamically different situations are possible, in two of these the gas layer is warped. The morphology of elliptical radio galaxies with dust lanes such as NGC 5128 (Cen A) and M84 can be understood on the basis of this model; transient phenomena are not required. © Royal Astronomical Society.
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页码：303 / &
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