Hostname: page-component-745bb68f8f-v2bm5 Total loading time: 0 Render date: 2025-01-13T00:13:20.446Z Has data issue: false hasContentIssue false
  • English
  • Français

Qualitative Analysis of the Stellar Content in LMC Clusters and Fields Using Objective Prism Schmidt Plates

Published online by Cambridge University Press:  26 July 2016

E. Kontizas ,
A. Dapergolas ,
E. Xiradaki  and
M. Kontizas
E. Kontizas
Affiliation:
Astronomical Institute, National Observatory of Athens, P.O. Box 20048, GR 118 10, Thission, Athens, Greece
A. Dapergolas
Affiliation:
Astronomical Institute, National Observatory of Athens, P.O. Box 20048, GR 118 10, Thission, Athens, Greece
E. Xiradaki
Affiliation:
Section of Astrophysics, Astronomy and Mechanics, Department of Physics, National University of Athens, Panepistimiopolis GR157 83, Zographou, Athens, Greece
M. Kontizas
Affiliation:
Section of Astrophysics, Astronomy and Mechanics, Department of Physics, National University of Athens, Panepistimiopolis GR157 83, Zographou, Athens, Greece

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 distribution of spectral types in 64 LMC globular clusters and their adjoining fields have been studied.

Type
Part Ten: The Magellanic Clouds
Information
Symposium - International Astronomical Union , Volume 161: Astronomy from Wide-Field Imaging , 1994 , pp. 518 - 519
Copyright
Copyright © Kluwer 1994 

References

Kontizas, E., Kontizas, M. and Xiradaki, E., 1987. Astron. Astrophys. Suppl., 71, 575.Google Scholar
Kontizas, M., Kontizas, E. and Dapergolas, A., 1993. In preparation.Google Scholar
Kontizas, M., Morgan, D. H., Hadzidimitriou, D. and Kontizas, E., 1990. Astron. Astrophys. Suppl., 84, 257.Google Scholar