Far-infrared observations of Large Magellanic Cloud H II regions

Details Far-infrared observations of Large Magellanic Cloud H II regions Far-infrared observations of Large Magellanic Cloud H II regions

Aug 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978mnras.184..365w&link_type=abstract

Monthly Notices of the Royal Astronomical Society, vol. 184, Aug. 1978, p. 365-376.

Astronomy and Astrophysics

Astronomy

71

Far Infrared Radiation, H Ii Regions, Magellanic Clouds, Thermal Emission, Cosmic Dust, Hydrogen Ions, Light (Visible Radiation), Stellar Luminosity, Stellar Radiation

Scientific paper

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

Affiliated with

Also associated with

No associations

Rating

Far-infrared observations of Large Magellanic Cloud H II regions does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Far-infrared observations of Large Magellanic Cloud H II regions, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Far-infrared observations of Large Magellanic Cloud H II regions will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-945525