A model of a spiral galaxy with finite thickness

Huang Ying-liang
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Abstract

A first-order asymptotic solution (rapid phase variation) of the Poisson's equation for the three-dimensional potential in a special model is applied to a stationary, polytropic gas disk. After considering the vertical motion and the three-dimensional distributions of the physical parameters, a dispersion relation is derived. Numerical examples are calculated for the Schmidt model galaxy and for a thick galaxy to illustrate the variation of the wave number with height which may possibly account for certain observed facts about spiral arms.

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有限厚度螺旋星系的模型
将泊松方程的一阶渐近解(快速相位变化)应用于一个固定的多向气体盘。在考虑了垂直运动和物理参数的三维分布后,导出了色散关系。计算了Schmidt模型星系和厚星系的数值例子,以说明波数随高度的变化,这可能解释有关旋臂的某些观测事实。
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