한국우주과학회:학술대회논문집(한국우주과학회보) (Bulletin of the Korean Space Science Society)
- 한국우주과학회 2004년도 한국우주과학회보 제13권1호
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- Pages.26-26
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- 2004
The origin of CII emission in the Large Magellanic Cloud
초록
We compare the distribution of HI 21cm, HII 6563 AA, and CII 157.7 micron m line emission over the entire Large Magellanic Cloud (LMC). Bright CII emission is associated with HII regions and their surroundings, with a good correlation between CII and Halpha filaments. Diffuse CII emission is also detected in regions with no HII emission. We found a reasonably good correlation between the extended CII emission and HI emission. (omitted)
키워드