球状星团周围的潮汐尾
天体物理学
2007-09-05 v1
摘要
我们展示了在真实银河系（MW）势场中运动的星团的详细N体模拟结果。与银河系核球和星系盘的强烈相互作用导致了潮汐尾的形成，它们从星团的相对两侧延伸出来。它们的取向和形态可以很容易地用随动坐标系来解释。
引用
@article{arxiv.0709.0460,
title = {Tidal tails around globular clusters},
author = {M. Montuori and R. Capuzzo-Dolcetta and P. Di Matteo and P. Miocchi},
journal= {arXiv preprint arXiv:0709.0460},
year = {2007}
}
评论
2 pages, 2 figures, presented at the Conference Pathways Through an Eclectic Universe, Tenerife, Spain, 3rd to 27th April, 2007, ASP Conf. Ser., in press