期刊
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
卷 387, 期 3, 页码 1248-1252出版社
OXFORD UNIV PRESS
DOI: 10.1111/j.1365-2966.2008.13323.x
关键词
methods : analytical; methods : N-body simulations; galaxies : kinematics and dynamics; galaxies : star clusters
We examine the longitudinal distribution of the stars escaping from a cluster along tidal tails. Using both theory and simulations, we show that, even in the case of a star cluster in a circular galactic orbit, when the tide is steady, the distribution exhibits maxima at a distance of many tidal radii from the cluster.
作者
我是这篇论文的作者
点击您的名字以认领此论文并将其添加到您的个人资料中。
推荐
暂无数据