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Main Sequence Photometry of Kron 3

Published online by Cambridge University Press:  04 August 2017

R. M. Rich ,
J. R. Mould  and
G.S. Da Costa
R. M. Rich
Affiliation:
Palomar Observatory, California Institute of Technology
J. R. Mould
Affiliation:
Palomar Observatory, California Institute of Technology
G.S. Da Costa
Affiliation:
Yale University Observatory

Abstract

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The globular cluster Kron 3 in the Small Magellanic Cloud presents an interesting opportunity to study stellar evolution in a population of intermediate age populous enough to contain many stars in short-lived phases of their evolution. The cluster lies approximately two degrees west of the body of the SMC and just outside the tidal radius of the Galactic globular cluster 47 Tuc.

Type
Magellanic Cloud Clusters
Information
Symposium - International Astronomical Union , Volume 108: Structure and Evolution of the Magellanic Clouds , 1984 , pp. 45 - 46
Copyright
Copyright © Reidel 1984