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In this paper we present a study and comparison of the star formation rates (SFRs) in the fields around NGC 1898 and NGC 2154, two intermediate‐age star clusters located in very different regions of the Large Magellanic Cloud (LMC). We also derive ages for NGC 1898, and seven minor clusters which happen to fall in the field of NGC 1898, for which basic parameters were previously unknown. We do not...
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