VizieR

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

VizieR

  
J/AJ/134/926
  Chemical composition of V2314 Oph (Kim+, 2007)
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2007AJ....134..926K
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Objects
Post annotation 		  
1.J/AJ/134/926/table4Lines of other elements in the spectrum of V2314 Oph (111 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)
  Ion  Ion identification code (e.g. FeI = 26.00) (phys.atmol.element)
  Wave 0.1nm Wavelength in Angstroms (em.wl)
  log(gf) [-] Log of the oscillator strength (phys.atmol.oscStrength)
  Elow eV Excitation energy (phys.atmol.excitation)
  DlogN [-] Log of abundance difference from solar (Note 2)   (phys.abund)
  logN [-] Log of V2314 Oph element abundance (phys.abund)
  logNSun [-] (n) Log of solar element abundance (Note 2)   (phys.abund)
  bld   [0,1] Level of synthetic spectrum line blending in V2314 Oph (Note 3)   (meta.note)
  bldSun  (n) [0,1] Level of synthetic spectrum line blending in Sun (Note 3)   (meta.note)
  Depth   [0,1] Synthetic spectrum line depth in V2314 Oph (phys.absorption.opticalDepth;spect.line)
  DepthSun  (n) [0,1] Synthetic spectrum line depth in Sun (phot.flux.density;arith.ratio)
  dlog(gf) [-] Change of log of the abundance for atmosphere model with log(gf) shifted by -0.2dex (stat.fit.param)
  dTeff [-] Change of log of the abundance for atmosphere model with Teff shifted by +100K (stat.fit.param)

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