M51星系盘上星团光度函数的变化
天体物理学
2007-05-23 v1
摘要
我们研究了M51中星团的光度函数（LF）。将观测到的LF与人工星团群体产生的LF进行比较表明，星团存在一个上限质量，并且该上限和/或星团瓦解随星系中心距离而变化。
引用
@article{arxiv.astro-ph/0609018,
title = {Variation of the cluster luminosity function across the disk of M51},
author = {M. R. Haas and M. Gieles and R. A. Scheepmaker and S. S. Larsen and H. J. G. L. M. Lamers and N. Bastian},
journal= {arXiv preprint arXiv:astro-ph/0609018},
year = {2007}
}
备注
2 pages, no figures. To appear in "Mass loss from stars and the evolution of stellar clusters". Proc. of a workshop held in honor of Henny Lamers, Lunteren, The Netherlands, May 29 - June 1, 2006. Editors Alex de Koter, Linda Smith and Rens Waters (San Francisco: ASP)