The UM/CTIO Magellanic Cloud Emission-line Survey

被引：55
|
作者：
Smith, RC [1 ]
机构：
[1] Univ Michigan, Dept Astron, Ann Arbor, MI 48109 USA
来源：
PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF AUSTRALIA | 1998年 / 15卷 / 01期
关键词：
Magellanic Clouds; surveys; ISM; general;
D O I：
10.1071/AS98163
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
The Magellanic Clouds are unique in providing us with sites to study the interstellar medium (ISM) and its components at all scales. To promote the pursuit of such studies, we have begun the Magellanic Cloud Emission-line Survey (MCELS), a deep imaging survey of both of these nearby galaxies in the emission of H alpha, [S II], and [O III]. The emission-line images will be used in detailed optical and multiwavelength studies of HII regions, supernova remnants, planetary nebulae, superbubbles, and supergiant shells. Together with parallel surveys at other wavelengths, this survey will provide the foundation upon which to build a deeper understanding of the ISM in the Clouds and other galaxies, from small scales (similar to 1 pc) all the way up to global scales.
引用
收藏
页码：163 / 164
页数：2
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