VizieR

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VizieR

  
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)
2.J/A+A/490/151/modelsSummary of models (3140 rows)

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

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 (i)indexed column
  (2)IMF (char) [SK] Salpeter or Kroupa IMF (meta.id;stat.fit)
  (2)r (char) [r-] "r" if model includes remnants (meta.id;stat.fit)
  (2)L (char) [L-] "L" if model includes preferential loss of low-mass stars (meta.id;stat.fit)
  (2)tD Myr Dissolution timescale (stat.param)
  (2)logMo [solMass]Initial mass of the cluster (log scale) (phys.mass)
  (2)logMf [solMass]Final mass of the cluster (at tf) (phys.mass)
  (2)logtf [yr] Final time (log scale) (time.age)
  (2)File (char) File name containing the model (meta.id;stat.param;meta.modelled)
  (2)Record  Starting record number of the model in File (meta.record)
  (2)Plot (char) Plot the evolution for this model (meta.ref.url)

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