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J/MNRAS/491/3251
  Globular clusters in the inner Galaxy (Perez-Villegas+, 2020)
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2020MNRAS.491.3251P
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Post annotation 		img(gal)
1.J/MNRAS/491/3251/table5Membership probability for different bar pattern speed (78 rows)

Simple ConstraintList Of Constraints
 
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)
  Bulge40 % Probability of the cluster to be part of the bulge for Ωb=40km/s/kpc (stat.probability)
  Disk40 % Probability of the cluster to be part of the disk for Ωb=40km/s/kpc (stat.probability)
  Haloi40 % Probability of the cluster to be part of the inner halo for Ωb=40km/s/kpc (stat.probability)
  Haloo40 % Probability of the cluster to be part of the outer halo for Ωb=40km/s/kpc (stat.probability)
  Bulge45 % Probability of the cluster to be part of the bulge for Ωb=45km/s/kpc (stat.probability)
  Disk45 % Probability of the cluster to be part of the disk for Ωb=45km/s/kpc (stat.probability)
  Haloi45 % Probability of the cluster to be part of the inner halo for Ωb=45km/s/kpc (stat.probability)
  Haloo45 % Probability of the cluster to be part of the outer halo for Ωb=45km/s/kpc (stat.probability)
  Bulge50 % Probability of the cluster to be part of the bulge for Ωb=50km/s/kpc (stat.probability)
  Disk50 % Probability of the cluster to be part of the disk for Ωb=50km/s/kpc (stat.probability)
  Haloi50 % Probability of the cluster to be part of the inner halo for Ωb=50km/s/kpc (stat.probability)
  Haloo50 % Probability of the cluster to be part of the outer halo for Ωb=50km/s/kpc (stat.probability)

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