银河动力学的三个贡献：远距离星系运动学、质量与 M/L 比值演化
天体物理学
2007-05-23 v1
摘要
1) 旋转曲线与银河系 M/L 演化至 z=0.4 (Bershady、Haynes、Giovanelli、& Andersen) 2) 单爆发星系质量估计：线宽与近红外光度比较 (Jangren、Bershady、& Gronwall) 3) 基于全场光谱学的星系运动学 (Andersen、Bershady)
引用
@article{arxiv.astro-ph/9812020,
title = {Three contributions to Galaxy Dynamics: distant galaxy kinematics, mass, and M/L},
author = {M. A. Bershady and A. Jangren and D. R. Andersen and M. P. Haynes and R. Giovanelli and C. Gronwall},
journal= {arXiv preprint arXiv:astro-ph/9812020},
year = {2007}
}
备注
8 pages, 5 embedded figures, to appear in the Proceedings of Galaxy Dynamics, ASP Conference Series, eds. D.R. Merritt, M. Valluri, J.A. Sellwood