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The SMC Cluster NGC330

Published online by Cambridge University Press:  14 August 2015

Kenneth A. Janes  and
Bruce W. Carney
Kenneth A. Janes
Affiliation:
Boston University
Bruce W. Carney
Affiliation:
Department of Terrestrial Magnetism, Carnegie Institution of Washington

Extract

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The cluster NGC330 is compact, populous, and one of the brightest objects in the Small Magellanic Cloud. Because of its size and its large number of blue supergiants, it has been referred to as a “blue globular”, as have several other clusters in the Clouds. To learn whether this appellation is more than superficial, we have undertaken a general study of the cluster. We have obtained DDO photometry, photoelectric and photographic UBV photometry, and low-dispersion spectroscopy of stars in and near the cluster. We report here our preliminary analyses of the data.

Type
August 29 Open And Globular Clusters
Information
Symposium - International Astronomical Union , Volume 85: Star Clusters , 1980 , pp. 349 - 352
Copyright
Copyright © Reidel 1980 

References

Arp, H.: 1959, Astron. J. 64, 254.CrossRefGoogle Scholar
Robertson, J.W.: 1974, Astron. Astrophys. Suppl. 15, 261.Google Scholar
Searle, L., and Zinn, R.: 1978, Astrophys. J. 225, 357.CrossRefGoogle Scholar