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A BV Photometric Study of Star Clusters in Two Selected Regions of the SMC

Published online by Cambridge University Press:  04 August 2017

Gonzalo Alcaino  and
William Liller
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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We are deriving BV color-magnitude diagrams of star clusters in two selected regions in the SMC. These zones, characterized by the presence of a high density of star clusters, are centered at the 1981 coordinates for region 1: (RA: 1h, Dec −73°08′), and for region 2: (RA: 1h 10m.33, Dec −73°00′). See Figure 1 for their identification relative to the SMC.

Type
Magellanic Cloud Clusters
Information
Symposium - International Astronomical Union , Volume 108: Structure and Evolution of the Magellanic Clouds , 1984 , pp. 51 - 52
Copyright
Copyright © Reidel 1984 

References

Walker, M. F.: 1972, Mon. Not. Roy. Astron. Soc. 159, p. 379.Google Scholar