CaltechAUTHORS
Published 1986 | Version Published
Book Section - Chapter Open

The Structure of Globular Clusters

Creators

  • 1. ROR icon University of California, Berkeley

Contributors

Abstract

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-mode1–1ike clusters.

Additional Information

© 1986 IAU.

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Published - 1986IAUS__118__281D.pdf

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1986IAUS__118__281D.pdf

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Additional details

Identifiers

Eprint ID
97563
DOI
10.1007/978-94-010-9433-7_53
Resolver ID
CaltechAUTHORS:20190731-144844274

Related works

Describes
10.1007/978-94-010-9433-7_53 (DOI)
http://adsabs.harvard.edu/abs/1986IAUS..118..281D (URL)

Dates

Created
2019-07-31
Created from EPrint's datestamp field
Updated
2021-11-16
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Caltech Custom Metadata

Series Name
International Astronomical Union
Series Volume or Issue Number
118