VizieR

CfA VizieR . ADAC VizieR . Cambridge (UK) VizieR . IUCAA VizieR . INASAN VizieR .

VizieR

  
J/A+A/701/A29
  Photoionization models (Peluso+, 2025)
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2025A&A...701A..29P
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1.J/A+A/701/A29/agngridsPhotoionization models generated using the CLOUDY v17.02 code, ionization comes from the radiation of an active galactic nucleus (AGN) (112 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)
  nH cm-3 [100] Gas density (phys.columnDensity)
  alpha   [-2.0] AGN continuum slope (Note 1)   (stat.fit.param)
  dg   [-0.52] Dust-to-gas ratio (Note G2)   (phys.mass;arith.ratio)
  logU   [-4.0/-0.5] Ionization parameter (Note G3)   (phys.ionizParam)
  logZ   [-1.0/0.7] Gas-phase metallicity (Note G4)   (phys.abund.Z)
  OIIa  Predicted emission line flux relative to H{beta} for [OII]{lambda}3726 (phot.flux;arith.ratio;spect.line)
  OIIb  Predicted emission line flux relative to H{beta} for [OII]{lambda}3729 (phot.flux;spect.line;arith.ratio)
  OII  Predicted emission line flux relative to H{beta} for [OII]{lambda}{lambda}3726,29 (phot.flux;arith.ratio;spect.line)
  Ha  Predicted emission line flux relative to H{beta} for H{alpha}{lambda}6563 (phot.flux;spect.line;arith.ratio)
  OIIIb  Predicted emission line flux relative to H{beta} for [OIII]{lambda}5007 (phot.flux;spect.line;arith.ratio)
  OI  Predicted emission line flux relative to H{beta} for [OI] {lambda}6300 (phot.flux;arith.ratio;spect.line)
  NIIb  Predicted emission line flux relative to H{beta} for [NII] {lambda}6584 (phot.flux;arith.ratio;spect.line)
  SIIa  Predicted emission line flux relative to H{beta} for [SII] {lambda}6716 (phot.flux;arith.ratio;spect.line)
  SIIb  Predicted emission line flux relative to H{beta} for [SII] {lambda}6731 (phot.flux;arith.ratio;spect.line)
  SII  Predicted emission line flux relative to H{beta} for [SII] {lambda}{lambda}6716,31 (phot.flux;spect.line;arith.ratio)

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