Age Determination of HII Regions of the Large Magellanic Cloud and Small Magellanic Cloud

Details Age Determination of HII Regions of the Large Magellanic Cloud and Small Magellanic Cloud Age Determination of HII Regions of the Large Magellanic Cloud and Small Magellanic Cloud

Sep 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984iaus..108..383c&link_type=abstract

Structure and Evolution of the Magellanic Clouds, Proceedings of IAU Symposium No. 108, held 5-8 September 1983 in Tübingen, Wes

Physics

2

Scientific paper

Models of H II regions in the MC were constructed by assuming an initial
burst of star formation. Effects of various initial mass functions and
upper stellar mass limits are taken into account and stellar evolution
with and without mass loss is considered. Limits for H II region ages
are in the range 1×106 - 4×106yr.

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