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Far-infrared observations of Large Magellanic Cloud H II regions

  • Werner M
  • Becklin E
  • Gatley I
  • et al.
Monthly Notices of the Royal Astronomical Society (1978) 184(2) 365-376
DOI: 10.1093/mnras/184.2.365
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Abstract

Far-infrared emission has been measured from four Large Magellanic CloudH II regions: the 30 Doradus nebula, MC75, MC76 and MC77. Thefar-infrared radiation is thermal emission from dust heated bystarlight. The results show that the LMC H II regions, like H II regionsin the Galaxy, have far-infrared luminosities comparable to the totalluminosity of their exciting stars.

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APA

Werner, M. W., Becklin, E. E., Gatley, I., Ellis, M. J., Hyland, A. R., Robinson, G., & Thomas, J. A. (1978). Far-infrared observations of Large Magellanic Cloud H II regions. Monthly Notices of the Royal Astronomical Society, 184(2), 365–376. https://doi.org/10.1093/mnras/184.2.365

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