通过红外观测研究银河系亮蓝变星的性质
太阳与恒星天体物理
2010-12-15 v1
摘要
近期对银道面的红外巡天揭示了大量亮蓝变星候选体。为验证这些分类，我们开展了一项长期的光谱和测光监测计划，并辅以定制的非局部热动平衡模型大气分析。本文简要概述了该计划的若干方面，重点展示了在近红外光谱窗口中对亮蓝变星进行证认、分类和定量分析的前景。
引用
@article{arxiv.1012.2997,
title = {Investigating the properties of Galactic Luminous Blue Variables via IR observations},
author = {J. S. Clark and A. Arkharov and V. Larionov and B. Ritchie and P. Crowther and F. Najarro},
journal= {arXiv preprint arXiv:1012.2997},
year = {2010}
}
备注
5 pages, 3 figures, to appear in the proceedings of the 39th Liege International Astrophysical Colloquium on "The multi-wavelength view of hot, massive stars", Liege, 12-16 July 2010