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NGC 6723

Published online by Cambridge University Press:  25 April 2016

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Extract

A preliminary investigation of this cluster was carried out by Gascoigne and Ogston (1963). They found that the cluster is probably a disc type globular on the basis of the c-m diagram down to the horizontal branch and its integrated spectral type (G2).

Type
Contributions
Information
Publications of the Astronomical Society of Australia , Volume 1 , Issue 1 , January 1967 , pp. 16
Copyright
Copyright © Astronomical Society of Australia 1967

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References

Eggen, O. J., 1961.—Roy. Obs. Bull., No. 29.Google Scholar
Gascoigne, S. C. B., and Ogston, F. A., 1963.—Observatory 83, 64.Google Scholar
Sandage, A. R., and Katem, B., 1964.—Ap. J. 139, 1088.Google Scholar
Sandage, A., and Smith, L. L., 1966.—Ap. J. 144, 886.Google Scholar
Sandage, A., and Walker, M. F., 1966.—Ap. J. 143, 313.CrossRefGoogle Scholar
Tifft, W. G., 1963.—M.N.R.A.S. 126, 209.CrossRefGoogle Scholar
Wildey, R. L., 1961.—Ap. J. 133, 430.Google Scholar