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J/A+A/490/151
  Photometric evolution of star clusters models (Kruijssen+, 2008)
model
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1.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)

 
Query by Constraints constraints help applied on Columns (Output Order: + - )
ShowSortColumn  Constraint Explain   (UCD)
  recno  Record number assigned by the VizieR team. Should Not be used for identification. (meta.record)
  Type (char) [LT] (L)uminous cluster mass (qevlum) or (T)otal cluster mass (qevtot) (meta.code)
  Z  Initial metallicity (phys.abund.Z)
  Mass solMass Initial maximum stellar mass (Note 1)   (phys.mass)
  aS  Salpeter IMF aev parameter (stat.param)
  bS  Salpeter IMF bev parameter (stat.param)
  cS  Salpeter IMF cev parameter (stat.param)
  aK  Kroupa IMF aev parameter (stat.param)
  bK  Kroupa IMF bev parameter (stat.param)
  cK  Kroupa IMF cev parameter (stat.param)
  Dir (char) (i) Name of the subdirectory containing the model files (Note 2)   (meta.id;meta.file)

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