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The structure of globular clusters

Published online by Cambridge University Press:  04 August 2017

S. Djorgovski ,
I. R. King ,
C. Vuosalo ,
A. Oren  and
H. Penner
S. Djorgovski
Affiliation:
Astronomy Department University of California Berkeley, CA 94720, U.S.A.
I. R. King
Affiliation:
Astronomy Department University of California Berkeley, CA 94720, U.S.A.
C. Vuosalo
Affiliation:
Astronomy Department University of California Berkeley, CA 94720, U.S.A.
A. Oren
Affiliation:
Astronomy Department University of California Berkeley, CA 94720, U.S.A.
H. Penner
Affiliation:
Astronomy Department University of California Berkeley, CA 94720, U.S.A.

Abstract

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We report the preliminary results of a CCD surface photometry survey of a large fraction of all known Galactic globular clusters. About 1/5 of all surveyed clusters show a characteristic post-core-collapse (PCC) morphology. The PCC clusters are on average closer to the Galactic center than the King-model-like clusters.

Type
II. Photometric Research Programmes
Information
Symposium - International Astronomical Union , Volume 118: Instrumentation and Research Programmes for Small Telescopes , 1986 , pp. 281 - 282
Copyright
Copyright © Reidel 1986 

References

Djorgovski, S. and King, I.R. 1984, Ap. J. Lett. 277, L49.CrossRefGoogle Scholar
Goodman, J. and Hut, P., (eds.) 1985, Proceedings of the I.A.U. Symposium #113, “Dynamics of Star Clusters”. Dordrecht: D. Reidel.CrossRefGoogle Scholar