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  J/A+A/490/151
 Photometric evolution of star clusters models (Kruijssen+, 2008)
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    J/A+A/490/151/table1*Fitting values for a, b and c for the luminous fractional cluster mass decrease due to stellar evolution. (Note) (10 rows)
    J/A+A/490/151/modelsSummary of models (3140 rows)

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