VizieR

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

VizieR

  
J/PASP/124/401
  Chemical composition of BE Lyn (Kim+, 2012)
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2012PASP..124..401K
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Post annotation 		  
1.J/PASP/124/401/table1Iron Lines in Spectrum of BE Lyn (147 rows)
2.J/PASP/124/401/table2Lines of chemical elements in spectrum of BE Lyn (except iron) (242 rows)
3.J/PASP/124/401/refsReferences (22 rows)
4.J/PASP/124/401/table3Mean abundances of chemical elements in atmosphere of BE Lyn (34 rows)

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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+2)lambda 0.1nm Wavelength (em.wl)
  (1+4)Ion (char) Ion (Fe I or Fe II) (phys.atmol.ionStage)
  (1+2)loggf [-] Oscillator strength (phys.atmol.oscStrength)
  (1+2)Elow eV Energy of low level (phys.energy;phys.atmol.level)
  (1)EW 0.1pm Equivalent width (in mÅ) (spect.line.eqWidth)
  (1+4)logN [-] Iron abundance (in the scale of logN(H)=12) (phys.abund)
  (2)Ion  Ion numerial code (FeI=26.00) (phys.atmol.ionStage)
  (2)r_loggf  Reference for loggf, in refs.dat file (meta.ref;pos.frame)
  (2+4)DlogN [-] Differential abundance, Be Lyn - Sun (in the scale of logN(H)=12) (phys.abund)
  (2)logN* [-] BE Lyn abundance (in the scale of logN(H)=12) (phys.abund)

ALL cols		    
 (i)indexed column
  (2)logNS [-] (n) Sun abundance (in the scale of logN(H)=12) (phys.abund)
  (2)Bl*  (n) Be Lyn level of blending of the line in the synthetic spectra (1 = clean line, 0.0 = strong blended line) (meta.code)
  (2)n_Bl* (char) [h] h for hfs: hyperfine splitting (meta.note)
  (2)BlS  (n) Sun level blending of the line in the synthetic spectra (1 = clean line, 0.0 = strong blended line) (meta.code)
  (2)n_BlS (char) [h] h for hfs: hyperfine splitting (meta.note)
  (2)D*  BE Lyn depth of the line in synthetic spectra (phot.flux.density;arith.ratio)
  (2)DS  (n) Sun depth of the line in synthetic spectra (phot.flux.density;arith.ratio)
  (2)dA(T) [-] Correction for abundance, by an effective temperature decrease of 200K (arith.factor)
  (2)dA(g) [-] Correction for abundance, by a gravity increase of 0.3dex (arith.factor)
  (2)dA(vt) [-] Correction for abundance, by a microturbulent velocity increase of 0.5km/s (arith.factor)
  (2)D  Depth of the line in convoluted synthetic spectra (phot.flux.density;arith.ratio)
  (2)dD1  Correction to the best depth of the line in the synthetic spectrum found by changing the abundance of the investigated chemical element by -0.5dex (arith.factor)
  (2)dD2  Correction to the best depth of the line in the synthetic spectrum found by changing the abundance of the investigated chemical element by +0.5dex (arith.factor)

ALL cols		    
(n) indicates a possible blank or NULL column(i)indexed column
  (3)Ref  Reference number (meta.id;meta.main)
  (3)Com (char) Reference (meta.ref;pos.frame)
  (4)Z  Atomic number (meta.id;meta.main)
  (4)n  Number of line used (meta.number)
  (4)e_DlogN [-] (n) rms uncertainty on DlogN (stat.error)
  (4)DlogN1 [-] Relative abundance in BL Lyn atmosphere, effective temperature increased by 100K (phys.abund)
  (4)e_DlogN1 [-] (n) rms uncertainty on DlogN1 (stat.error)
  (4)DlogN2 [-] Relative abundance in BL Lyn atmosphere, surface gravity decreased by 0.3dex (phys.abund)
  (4)e_DlogN2 [-] (n) rms uncertainty on DlogN2 (stat.error)
  (4)DlogN3 [-] Relative abundance in BL Lyn atmosphere, microturbulent velocity increased by 0.5km/s (phys.abund)
  (4)e_DlogN3 [-] (n) rms uncertainty on DlogN3 (stat.error)
  (4)e_logN [-] (n) rms uncertainty on logN (stat.error)
  (4)logN1 [-] Absolute abundance in BL Lyn atmosphere, effective temperature increased by 100K (phys.abund)

ALL cols		    
(n) indicates a possible blank or NULL column(i)indexed column
  (4)e_logN1 [-] (n) rms uncertainty on logN1 (stat.error)
  (4)logN2 [-] Absolute abundance in BL Lyn atmosphere, surface gravity decreased by 0.3dex (phys.abund)
  (4)e_logN2 [-] (n) rms uncertainty on logN2 (stat.error)
  (4)logN3 [-] Absolute abundance in BL Lyn atmosphere, microturbulent velocity increased by 0.5km/s (phys.abund)
  (4)e_logN3 [-] (n) rms uncertainty on logN3 (stat.error)

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