Tucana 矮星系
天体物理学
2007-05-23 v1
摘要
present deep CCD 光度测量 (NTT, HST 数据)，下至 V=27.5。推导出距离模和金属丰度，并估计星系的年龄。
引用
@article{arxiv.astro-ph/9511144,
title = {The Tucana dwarf galaxy},
author = {Marco Castellani and Gianni Marconi and Roberto Buonanno},
journal= {arXiv preprint arXiv:astro-ph/9511144},
year = {2007}
}
备注
4 pages, 3 Postscript figures. To appear in The Proceedings for the "Formation of the Galactic Halo...Inside and Out"