M51的新测光研究
天体物理学
2009-10-31 v1
摘要
一种新技术被用于从高信噪比多色测光数据中推导相互作用星系NGC5194和NGC5195中星族的消光和年龄。提出了相互作用的新演化情景。
引用
@article{arxiv.astro-ph/9906352,
title = {A New Photometric Look at M51},
author = {Vladas Vansevicius},
journal= {arXiv preprint arXiv:astro-ph/9906352},
year = {2009}
}
备注
6 pages, 4 figures, to appear in "The Evolution of galaxies on Cosmological timescales", Ap&SpSci, in press