摘要
Coma团是离我们最近的典型富星系团之一。对此，人们积累了丰富的观测资料，并且进行了广泛深入的研究。在本文中着重介绍有关Coma团的成员判定、结构、光度函数、动力学和次结构等方面的研究情况，并简单介绍目前的最新研究动态。
Coma, which is the nearest One to us, is a typical regular rich galaxy cluster. Over the years, various observational data of this cluster have been collected, and many problems have been discussed in depth. In this paper, we present the studies about the Coma's membership, structure, luminosity function, dynamics and substructures. We also introduce the focus of recent studies.
出处
《天文学进展》
CSCD
北大核心
1995年第2期152-163,共12页
Progress In Astronomy
基金
国家自然科学基金
