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J/MNRAS/432/2746
  POPSTAR models. III. Young star clusters (Garcia-Vargas+, 2013)
model/cluster
Post annotation
  
1.J/MNRAS/432/2746/table1Computed radii for the modelled stellar clusters of all ages and metallicities, for ne=10 and 100cm–3 (4116 rows)

 
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ShowSortColumn  Constraint Explain   (UCD)
  recno  Record number assigned by the VizieR team. Should Not be used for identification. (meta.record)
  ne cm-3 [10/100] Electron density of the stellar cluster ISM used for CLOUDY models (10 or 100) (phys.density;phys.electron)
  Z   [0.0001/0.05] Total abundance of the stellar cluster (phys.abund)
  logt [yr] [5/8] Log of age of the stellar cluster (time.age)
  Mass 10+4Msun [1.2/20] Initial total cluster mass (phys.mass)
  Rin pc [4.7/445.3] Inner radius of the HII region (phys.size.radius;obs.field)
  deltaR pc Shell thickness of the HII region (src.morph.param)
  Rout pc [6/8597] External radius (observed) of the HII region (phys.size.radius;obs.field)

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