Hot gas in the large magellanic cloud
The Large Magellanic Cloud (LMC) o ers an excellent laboratory to studythe physical structure of the interstellar medium (ISM) because of its proximity,nearly face-on orientation, and small foreground and internal extinction. Opticaland radio surveys of the LMC ISM have revealed interstellar structu...
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| 發表在: | Revista Mexicana de Astronomía y Astrofísica |
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| 主要作者: | |
| 格式: | Artigo |
| 語言: | Inglês |
| 出版: |
Universidad Nacional Autónoma de México
2000
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| 主題: | |
| 在線閱讀: | https://www.redalyc.org/articulo.oa?id=57100967 |
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