Chemical compositions of Magellanic Clouds' HII regions based on photoelectric spectrophotometry
L H Aller1, S J Czyzak, C D Keyes
1Department of Astronomy, University of California, Los Angeles, California 90024.
Abstract:
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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