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central condensation
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  central condensation
This may indicate that the subcluster is moving toward a central condensation of faint galaxies in the Coma cluster and a possible merger with it.
      
For the Galilean satellites we will determine second degree and order gravity harmonics that will yield new information on the central condensation and likely composition of material within these giant satellites (Hubbard and Anderson, 1978).
      
It is found that as the central degeneracy parameter is increased, the central condensation in general decreases and, hence, the eccentricity of the configuration decreases.
      
Models have been computed for varying degrees of central degeneracy and the effect of the magnetic field on the various parameters, e.g., mass, central condensation, moment of inertia, and oblateness has been looked into.
      
The effect of magnetic field on the various structural parameters, e.g., mass, central condensation, moment of inertia, and oblateness has been computed for different values of the central degeneracy of the model.
      
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In this paper we have investigated numerically a model of three-dimensional gravitating system of colliding particles, called "the model of ellipsoid", in which particles are moving in the gravitational field of a central rotational ellipsoid body and interact through inelastic collisions. We have given a program of numerical simulation of collisional evolution for this model in TQ-6 computer using BCY language. The results of calculation have proved Poincare's conclusion (1911). It is shown that after very...

In this paper we have investigated numerically a model of three-dimensional gravitating system of colliding particles, called "the model of ellipsoid", in which particles are moving in the gravitational field of a central rotational ellipsoid body and interact through inelastic collisions. We have given a program of numerical simulation of collisional evolution for this model in TQ-6 computer using BCY language. The results of calculation have proved Poincare's conclusion (1911). It is shown that after very fast flattening, the system reaches a quasi-equilibrium state and successively forms a disk of finite thickness. The disk spreads slowly and a central condensation is formed. It is coincided with real dish-like systems in the universe.

本文研究了一个三维引力碰撞质点系统的模型,即“椭球体模型”,其中所有质点是在一个旋转椭球中心体的引力作用下运动,且它们相互之间的碰撞是非弹性的。我们用BCY语言茬TQ-6机上对这个模型的碰撞演化进行数值模拟。计算结果证实了潘加莱的结论(1911)。计算表明该系统在很快变平以后,趋于准平衡态且形成一个有限厚度的盘。盘缓慢地伸展,中心凝聚逐渐形成。这些结论与宇宙中实际的盘状结构相符。

 
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