监控星形成区域中的水面母线
天体物理学
2009-11-10 v1
摘要
本文概述了我们监控计划中超过十年水母线数据分析。我们发现水母线发射通常取决于Young Stellar Object（YSO）的亮度以及星形成区域的几何结构。在YSO亮度超过几倍10^4 L_sol的阈值以下和以上，我们发现不同的母线特征。
引用
@article{arxiv.astro-ph/0407217,
title = {Monitoring water masers in star-forming regions},
author = {J. Brand and R. Cesaroni and G. Comoretto and M. Felli and F. Palagi and F. Palla and R. Valdettaro},
journal= {arXiv preprint arXiv:astro-ph/0407217},
year = {2009}
}
备注
9 pages, 1 table, 11 figures. Accepted for publ. in Ap&SpSci. Refereed contribution to "Dense Molecular Gas around Protostars and in Galactic Nuclei", European Workshop 2004 on Astronomical Molecules. Eds. Y. Hagiwara, W.A. Baan, H.J. van Langevelde