The Interstellar Medium in the Far Ultraviolet

被引：0
|
作者：
Howk, J. Christopher [1 ]
机构：
[1] Univ Notre Dame, Dept Phys, Notre Dame, IN 46556 USA
来源：
FUTURE DIRECTIONS IN ULTRAVIOLET SPECTROSCOPY | 2009年 / 1135卷
关键词：
Interstellar medium; Ultraviolet; SPECTROSCOPIC-EXPLORER SURVEY; LARGE-MAGELLANIC-CLOUD; O-VI EMISSION; MOLECULAR-HYDROGEN; FUSE SURVEY; ABSORPTION-LINES; OVI ABSORPTION; VELOCITY GAS; GALAXY; SIGHT;
D O I：
暂无
中图分类号：
O59 [应用物理学];
学科分类号：
摘要：
During its lifetime, FUSE produced a broad array of exciting results on the interstellar medium (ISM) of our own Milky Way and other galaxies. Some of its most important contributions in this area are in the physics of the highly ionized gas traced by 0 VI and of the molecular medium traced by the Lyman and Werner bands of H(2). I briefly note a few of these successes and discuss future directions and wishes for studying the ISM with next generation instruments.
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收藏
页码：73 / 76
页数：4
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