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J/MNRAS/492/895
  Ultracompact HII regions extended emission (de la Fuente+, 2020)
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2020MNRAS.492..895D
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Post annotation 		img(gal)
1.J/MNRAS/492/895/table6Results on the energetics for the initial sample (39 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) Name of the HII region (GLLL.ll+BB.bb) (meta.id;meta.main)
  LIRAS 10+4Lsun Total luminosity measured via IRAS fluxes (phys.luminosity)
  logN*c [s-1] Logarithm of the ionizing photon rate N*c (Note G2)   (phys.luminosity)
  SpTypeI (char) Spectral type from IRAS observations (src.spType)
  VLA (char) [CD] VLA configuration (instr.setup)
  logN**c [s-1] Logarithm of the ionizing photon rate N**c (Note G3)   (phys.luminosity)
  SpTyper (char) Spectral type from radio observations (src.spType)
  fd(CD)  Fraction of UV photons absorbed by dust and hence without causing ionization for VLA C or D configuration (meta.number)
  fd(B)  (n) Fraction of UV photons absorbed by dust and hence without causing ionization for VLA B configuration (meta.number)
  r_fd(B)  (n) [1/2] Reference for fd(B) (Note G4)   (meta.ref;pos.frame)
  EElev  (n) [1/3] Different levels at which EE reduces the values of fd explaining the IR excess (Note 1)   (meta.code)

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