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Photometric Models for Globular Clusters from Population Synthesis
Published online by Cambridge University Press: 19 July 2016
Abstract
Integral fluxes (Bolometric and U, B, V) are computed in a completely theoretical frame in order to investigate the structural properties and stellar content of coeval stellar systems of various ages and metal abundance. Some results concerning the problem of the color gap in the distribution of the sample of Magellanic Cloud clusters are discussed.
- Type
- Chapter VIII. Poster Papers on Cluster Systems in Nearby Galaxies
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- Copyright © Kluwer 1988