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.
Photometric Models for Globular Clusters from Population Synthesis / CAPUZZO DOLCETTA, Roberto Angelo. - STAMPA. - (1988), pp. 559-560. (Intervento presentato al convegno Globular Cluster Systems in Galaxies tenutosi a Cambridge, MA, USA nel August 25-29, 1986).
Photometric Models for Globular Clusters from Population Synthesis
CAPUZZO DOLCETTA, Roberto Angelo
1988
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.File allegati a questo prodotto
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