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

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

Sep 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992cha%26a..16..239y&link_type=abstract

Chinese Astronomy and Astrophysics (ISSN 0275-1062) Translation., vol. 16, no. 3, p. 239-247.

Astronomy and Astrophysics

Astronomy

Cosmic Dust, Far Infrared Radiation, H Alpha Line, H Ii Regions, Magellanic Clouds, Infrared Astronomy Satellite, Milky Way Galaxy, Supernova Remnants

Scientific paper

From a comparison of the IRAS and smoothed H-alpha maps of the Magellanic Clouds, it was found that H-II regions with core-halo structure usually have higher F(60 microns)/F(H-alpha) ratios and probably emit more in the far infrared than do extended low-density H-II regions. This is consistent with the idea that the far infrared emission is mainly produced by dust within H-II regions.

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