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通信工程21年14期

卫星星系数目分布的研究进展
古慧
(西华师范大学,四川南充 637099)

摘  要:卫星星系存在于暗晕的子结构中,是暗物质晕等级成团的最直接的证据,为了解目前对卫星星系数目分布的研究现状,文章采用文献调查法对卫星星系的数目分布的研究进行了深入的调查,总结了卫星星系数目分布对中央星系的怪星质量的依赖,对星系所处的暗晕质量的依赖,对星系所处的大尺度结构的依赖,也总结了卫星星系的数目对中央星系的颜色和中央星系的形态的依赖。


关键词:中央星系;卫星星系;暗晕;颜色; 形态;环境



DOI: 10. 19850/j .cnki. 2096-4706.2021.14.009


中图分类号:PTP391; P15                                  文献标i只码:A                                         文章编号: 2096-4706 (2021) 14-0032-04


Research Progress on The Number Distribution of Satellite Galaxies

GU Hui
(China West Normal University, Nanchong  637099, China)

Abstract: Satellite galaxies exist in the substructure of dark halos, which is the most direct evidence of the hierarchical c1ustering  of dark matter halos. In order to understand 由e current research status of the number distribution of sate1lite galaxies, the paper uses the  literature survey method to deeply investigate the number distribution of sate1lite galaxies, and sununarizes the dependence of the number  dis仕ibution of satel1ite galaxies on the stellar mass of the central galaxy, and the dependence on the mass of the dark halo in which the  galaxy is located and on the large-scale structure in which the galaxy is located. It also summarizes the dependence of the number of  satellite galaxies on the color and shape of the central galaxy.
      Keywords: cen仕'al galaxy; satellite galaxy; dark matter halo; color; fonn; environment


参考文献:
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       作者简介:古慧(1997—),女,汉族,四川绵阳人,理学硕士在读,研究方向:天文学。