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A BVRI Photometric Study of Star Clusters in the Bok Region of the LMC

Published online by Cambridge University Press:  04 August 2017

Gonzalo Alcaino
Affiliation:
Instituto Isaac Newton, Ministerio de Educación de Chile, Santiago, Chile
William Liller
Affiliation:
Instituto Isaac Newton, Ministerio de Educación de Chile, Santiago, Chile

Extract

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The large number of star clusters in the Large Magellanic Cloud provides us with an excellent opportunity to understand well this neighboring galaxy. The large variety of integrated cluster colors present suggests a wide range in evolutionary stages, and several studies have established vague relationships between their location in the LMC and properties including color, total luminosity and metallicity.

Type
Magellanic Cloud Clusters
Copyright
Copyright © Reidel 1984 

References

Alcaino, G., and Liller, W.: 1982, Astron. Astrophys. 114, p. 213.Google Scholar