Observations of H II regions in the Magellanic Clouds

Details Observations of H II regions in the Magellanic Clouds Observations of H II regions in the Magellanic Clouds

Apr 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980esasp.157..205g&link_type=abstract

The second European International Ultraviolet Explorer (IUE) Conference, held 26-28 March 1980 in Tübingen, West Germany. Edited

Astronomy and Astrophysics

Astronomy

1

Cosmic Dust, H Ii Regions, Interstellar Extinction, Iue, Magellanic Clouds, Ultraviolet Astronomy, Absorption Spectra, Abundance, Carbon, Emission Spectra, Hydrogen, Nebulae

Scientific paper

International Ultraviolet Explorer observations of 5 positions in the 30 Doradus region and one in N79A in the Large Magellanic Cloud, and, N81 and N66 in the Small Magellanic Cloud were obtained. The C (III) line at 1909 A was present in almost all the objects. Dust scattered light was detected in 30 Dor and N66. A preliminary analysis of the abundances in N81 shows that carbon is underabundant by about a factor of 10.

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