Multi-wavelength view of the interstellar medium in the Large Magellanic Cloud

被引：0
|
作者：
Chu, YH [1 ]
机构：
[1] Univ Illinois, Dept Astron, Urbana, IL 61801 USA
来源：
PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF AUSTRALIA | 1998年 / 15卷 / 01期
关键词：
Magellanic Clouds; galaxies; ISM; general; structure; bubbles; supernova remnants;
D O I：
10.1071/AS98136
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
The Large Magellanic Cloud (LMC) has been surveyed in optical emission Lines, X-rays. radio continuum, Hr, and CO lines. These surveys provide views of the interstellar medium (ISM) in the LMC of unprecedented clarity, allowing us to study astrophysical processes and to examine the relationship among the different phases of the ISM. Multi-wavelength images are used to illustrate the physical structures of supernova, remnants, superbubbles, and supergiant shells, as well as the global interstellar structure of the LMC.
引用
收藏
页码：136 / 140
页数：5
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