Published 1986
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The Structure of Globular Clusters
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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-model–like clusters.
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© 1986 IAU.Attached Files
Published - Djorgovski1986_Chapter_TheStructureOfGlobularClusters.pdf
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Djorgovski1986_Chapter_TheStructureOfGlobularClusters.pdf
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- 97529
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- CaltechAUTHORS:20190730-143608851
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2019-08-01Created from EPrint's datestamp field
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- 118