Chemical Compositions of Magellanic Clouds' HII Regions Based on Photoelectric Spectrophotometry

Details Chemical Compositions of Magellanic Clouds' HII Regions Based on Photoelectric Spectrophotometry Chemical Compositions of Magellanic Clouds' HII Regions Based on Photoelectric Spectrophotometry

Dec 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977pnas...74.5203a&link_type=abstract

Proceedings of the National Academy of Sciences of the United States of America, Volume 74, Issue 12, pp. 5203-5206

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9

Scientific paper

Detailed line intensity measurements secured at Cerro Tololo Interamerican Observatory and corrected for interstellar extinction are presented for 19 HII regions in the Large Magellanic Cloud and 6 in the Small Magellanic Cloud. The elemental abundances derived by simple methods appear to be in good accord with those found by other observers. Detailed discussion is deferred to a later paper.

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