Hostname: page-component-5b777bbd6c-gcwzt Total loading time: 0 Render date: 2025-06-22T20:55:22.874Z Has data issue: false hasContentIssue false
  • English
  • Français

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

Published online by Cambridge University Press:  04 August 2017

Carla Cacciari
Carla Cacciari*
Affiliation:
ESTEC Astronomy Division, Villafranca, Spain

Extract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

The globular clusters NGC 1786 in LMC and NGC 121 and 330 in SMC have been observed in UV with IUE, both in the long and short wavelength range, in the low dispersion mode. The spectra show stellar component(s) superimposed on the cluster contributions.

Type
Magellanic Cloud Clusters
Information
Symposium - International Astronomical Union , Volume 108: Structure and Evolution of the Magellanic Clouds , 1984 , pp. 57 - 58
Copyright
Copyright © Reidel 1984 

References

Barbero, J. and Cassatella, A., 1983, Report to the IUE 3-Agency Meeting, London.Google Scholar
Kurucz, R.L., 1979, Astrophys. J. Suppl. 40, pp. 1.Google Scholar
Robertson, J.W., 1974, Astron. Astrophys. Suppl. 15, pp. 261.Google Scholar
Zinn, R., 1974, Astrophys. J. 193, pp. 593.Google Scholar