On the dispersion of star velocities in spiral galaxies

Huang Ke-liang, Huang Jie-hao, Peng Qiu-he
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引用次数: 1

Abstract

The variation with r of Cz2, the dispersion of velocities in z is obtained by direct integration. We also obtain the variation of the radial dispersion of velocities with r through the stability of the density wave in a three-dimensional dishlike galaxy. In the solar neighborhood, the theoretical values of Cr and Cz are in fair agreement with the observed values. And towards the centre of the galaxies, the value of Cr/Cz approaches 1.

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螺旋星系中恒星速度的色散
Cz2随r的变化,速度在z中的色散是通过直接积分得到的。我们还通过三维碟状星系中密度波的稳定性得到了速度的径向色散随r的变化。在太阳附近,Cr和Cz的理论值与观测值基本一致。在星系中心,Cr/Cz接近于1。
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Subject index Errata Author index Supernova remnants of known age and X-radiation The effect of an ellipsoidal distribution of star velocities on galactic density waves
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