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VizieR

  
J/A+A/683/A165
  Evaporation ages of young star clusters (Pelkonen+, 2024)
Post annotation
  
1.J/A+A/683/A165/table1Properties of the clusters considered in this study (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)
  Name (char) Cluster name (meta.id;meta.main)
  d pc Distance to the cluster (pos.distance)
  tCMD Myr CMD age from the PARSEC isochrones used in this work (time.age)
  E_tCMD Myr CMD age upper uncertainty (stat.error;stat.max)
  e_tCMD Myr CMD age lower uncertainty (stat.error)
  tDT Myr Dynamical traceback age (pos.parallax.dyn)
  E_tDT Myr Dynamical traceback age upper uncertainty (stat.error;stat.max)
  e_tDT Myr Dynamical traceback age lower uncertainty (stat.error)
  t*eva Myr Corrected evaporation age determined in this work (time.age)
  E_t*eva Myr Corrected evaporation age upper uncertainty (stat.error;stat.max)

ALL cols
    
 (i)indexed column
  e_t*eva Myr Corrected evaporation age lower uncertainty (stat.error)
  sigmap pc Observational error in position (stat.error;pos.distance;pos)
  sigmav km/s Observational error in velocity (stat.error;phys.veloc)
  R50 pc Core radius (phys.size.radius)
  Nstars  Number of stars used to obtain the CMD and dynamical traceback ages and the starting sample for the evaporation ages (meta.number)
  Ndiv  Number of divergent stars (meta.number)
  Neva  Number of evaporated star (meta.number)
  Neva70  Number of stars used to compute the evaporation age (meta.number)
  phieva  Correction factor of the evaporation age (see App. B) (arith.factor)
  sigmaeva  Correction factor uncertainty of the evaporation age (see App. B) (arith.factor)

ALL cols
    
 (i)indexed column
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