Disentangling Individual Star and Cluster Contributions in the IUE Spectra of Magellanic Cloud Globular Clusters
Abstract
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.
- Publication:
-
Structure and Evolution of the Magellanic Clouds
- Pub Date:
- September 1984
- DOI:
- 10.1017/S0074180900039930
- Bibcode:
- 1984IAUS..108...57C