VizieR

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VizieR

  
J/MNRAS/359/865
  Chemical composition of delta Sct (Yushchenko+, 2005)
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2005MNRAS.359..865Y
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Objects
Post annotation 		  
1.J/MNRAS/359/865/table3Iron lines in the Sct 2-m telescope of Peak Terskol Observatory spectrum of delta Sct (158 rows)
2.J/MNRAS/359/865/table4Lines of other elements in the 2-m telescope of Peak Terskol Observatory spectrum of delta Sct (432 rows)
3.J/MNRAS/359/865/table5Lines of chemical elements in the IUE spectrum of delta Sct (17 rows)

Simple ConstraintList Of Constraints
 
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Column  Constraint Explain   (UCD)
  (ALL)recno  Record number assigned by the VizieR team. Should Not be used for identification. (meta.record)
  (1)lambda 0.1nm Wavelength (em.wl)
  (1)Ion (char) Ion identification (Fe I or Fe II) (meta.id;phys.atmol.ionStage)
  (1)EW 0.1pm Equivalent width (spect.line.eqWidth)
   (ALL)loggf  Oscillator strength (phys.atmol.oscStrength)
   (ALL)Elow eV Excitation potential (phys.atmol.excitation)
   (ALL)logN  Abundance of the element in the atmosphere of delta Scuti, (log N(H)=12) (phys.abund)
  (2+3)Z  Atomic number and ionisation level (Fe I=26.00) (phys.atmol.element)
  (2+3)Lambda 0.1nm Wavelength of the line (em.wl)
  (2+3)Abun [Sun] (n) Abundance of the element in the atmosphere of delta Scuti with respect to the corresponding solar value (table4 only) (phys.abund)
  (2+3)logNsun  (n) Abundance of element in the atmosphere of the Sun (logN(H)=12) (table4 only) (phys.abund)

ALL cols		    
(n) indicates a possible blank or NULL column(i)indexed column
  (2+3)blend   [0/1] Level of blending of the line in the synthetic spectra of delta Scuti (Note 1)   (meta.note)
  (2+3)blSun  (n) [0/1] Level of blending of the line in the synthetic spectra of the Sun (table4 only) (Note 1)   (meta.note)
  (2+3)Depth   [0,1] Scuti depth in synthetic spectra (phot.flux.density;arith.ratio)
  (2+3)DepthS  (n) Sun depth in synthetic spectra (table4 only) (phot.flux.density;arith.ratio)
  (2+3)clogN1  (n) Correction to the abundance for a surface gravity decreased by 0.2dex (table4 only) (stat.fit.param)
  (2+3)clogN2  (n) Correction to the abundance for an effective temperature increased by 100K (table4 only) (stat.fit.param)

ALL cols		    
(n) indicates a possible blank or NULL column(i)indexed column
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