| 核盘晕星系相互作用的模拟研究 |
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| 引用本文： | 刘步林. 核盘晕星系相互作用的模拟研究[J]. 中国天文和天体物理学报, 1994, 0(4) |
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| 作者姓名： | 刘步林 |
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| 作者单位： | 中国科学院北京天文台 |
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| 摘 要： | 用一个星系相互作用数值模拟的综合三体模型，研究椭圆星系是否由盘星系合并而成。结果表明，主要取决于星系的盘面和星系运行轨道面的夹角。如果夹角不等于零，盘星系的相互作用是可能形成椭圆星系的，否则还是盘星系。
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| 关 键 词： | 数值模拟，三体模型，星系 |
The Numerical Simulation of Evolution of Interacting Galaxies with the Structure of Bulge,Disk and Halo |
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| LIU Bu-lin. The Numerical Simulation of Evolution of Interacting Galaxies with the Structure of Bulge,Disk and Halo[J]. Chinese Journal of Astronomy and Astrophysics, 1994, 0(4) |
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| Authors: | LIU Bu-lin |
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| Abstract: | perfect three-body model is used in the numerical simulation of interacting galaxies for studying whether merging disk galaxies make elliptical galaxy.It is showed by simulation that there are two possibilities:If the angle between disk plane and orbital plane of both galaxies do not equal to zero,it is possible that merging galaxies form a elliptical galaxy:if the angle equal to zero the merging galaxies will form a new disk galaxy. |
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| Keywords: | umerical simulation-three-body model-galaxies |
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