摘要
本文给出了利用视向速度、按最大似然原理对COMA星系团所作的成员判别的具体结果。对有关问题的讨论表明,我们所提出的判别星系团成员的方法是合理的。
The detailed results for membership of the Come cluster obtained from data of radial velocities based upon the maximum likelihood principle are given. It is shown from the discussions on problems concerned that the method we suggested for membership determination of clusters of galaxies is reasonable.
出处
《中国科学院上海天文台年刊》
1989年第10期43-56,共14页
Annals Shanghai Astronomical Observatory Chinese Academy of Sciences
