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A comparison of far infrared and H-alpha emission of H-II regions in the Magellanic clouds

✍ Scribed by Ye Tai-sheng


Publisher
Elsevier Science
Year
1992
Tongue
English
Weight
750 KB
Volume
16
Category
Article
ISSN
0275-1062

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l%e lauice spaeva of solid CCL,. monochnic pbasc II. have been rexxamin cd at h&x rgolution The greatly in- number of ob-cd paks IS POW cansistcnt with that cxpated for a crystal with 16 molczuls per unit cdl\_ if it is asum that only modes of a predo mmantly translatonal natu-c are de&ted.