Disentangling Individual Star and Cluster Contributions in the IUE Spectra of Magellanic Cloud Globular Clusters

Details Disentangling Individual Star and Cluster Contributions in the IUE Spectra of Magellanic Cloud Globular Clusters Disentangling Individual Star and Cluster Contributions in the IUE Spectra of Magellanic Cloud Globular Clusters

Sep 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984iaus..108...57c&link_type=abstract

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

Computer Science

2

Scientific paper

The globular clusters NGC 1786 in LMC and NGC 121 and 330 in SMC have
been observed in UV with the IUE. The spectra show stellar components
superimposed on the cluster contributions. The energy distributions for
the stars and clusters were separated by applying a new extraction
software. A short summary of the results is presented.

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