The Formation and Evolution of LMC Rich Star Clusters: NGC 1818

Details The Formation and Evolution of LMC Rich Star Clusters: NGC 1818 The Formation and Evolution of LMC Rich Star Clusters: NGC 1818

Jul 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998esoc...55..140j&link_type=abstract

NICMOS and the VLT: A New Era of High Resolution Near Infrared Imaging and Spectroscopy, Pula, Sardinia, Italy, June 26-27th 199

Physics

Scientific paper

The Large Magellanic Cloud (LMC) is uniquely suitable for the study of massive star clusters at all stages of evolution. By combining HST observations of these clusters with N-body models we hope to understand the origin and evolution of rich star clusters in our own Galaxy, in the LMC, and beyond. Here we give a brief overview of our large Cycle 7 HST project and present some preliminary results.

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