Physics
Scientific paper
Sep 1984
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984iaus..108...95m&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
3
Scientific paper
A model of the chemical evolution of the Magellanic Clouds including the
effects of stochastic star formation has been constructed. It is found
that the different chemical histories of the two Clouds may be related
to the fact that SMC has undergone several bursts of star formation
while a continuous star formation activity was present in LMC.
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