VizieR

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

VizieR

  
J/PASP/124/401
  Chemical composition of BE Lyn (Kim+, 2012)
ReadMe+ftp
2012PASP..124..401K
Similar Catalogs
Objects
Post annotation 		  
1.J/PASP/124/401/table2Lines of chemical elements in spectrum of BE Lyn (except iron) (242 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 numerial code (FeI=26.00) (phys.atmol.ionStage)
  lambda 0.1nm Wavelength (em.wl)
  loggf [-] Oscillator strength (phys.atmol.oscStrength)
  r_loggf  Reference for loggf, in refs.dat file (meta.ref;pos.frame)
  Elow eV Excitation potential (phys.atmol.excitation)
  DlogN [-] Differential abundance, Be Lyn - Sun (in the scale of logN(H)=12) (phys.abund)
  logN* [-] BE Lyn abundance (in the scale of logN(H)=12) (phys.abund)
  logNS [-] (n) Sun abundance (in the scale of logN(H)=12) (phys.abund)
  Bl*  (n) Be Lyn level of blending of the line in the synthetic spectra (1 = clean line, 0.0 = strong blended line) (meta.code)
  n_Bl* (char) [h] h for hfs: hyperfine splitting (meta.note)

ALL cols		    
(n) indicates a possible blank or NULL column(i)indexed column
  BlS  (n) Sun level blending of the line in the synthetic spectra (1 = clean line, 0.0 = strong blended line) (meta.code)
  n_BlS (char) [h] h for hfs: hyperfine splitting (meta.note)
  D*  BE Lyn depth of the line in synthetic spectra (phot.flux.density;arith.ratio)
  DS  (n) Sun depth of the line in synthetic spectra (phot.flux.density;arith.ratio)
  dA(T) [-] Correction for abundance, by an effective temperature decrease of 200K (arith.factor)
  dA(g) [-] Correction for abundance, by a gravity increase of 0.3dex (arith.factor)
  dA(vt) [-] Correction for abundance, by a microturbulent velocity increase of 0.5km/s (arith.factor)
  D  Depth of the line in convoluted synthetic spectra (phot.flux.density;arith.ratio)
  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)
  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
Adapt form
 Display your selection only Reset to default columns
usage  Display UCD1+    UCD1  
elapse time 0
→ Cite/acknowledge VizieR catalogue
→ Rules of usage of VizieR data

© UDS/CNRS

Contact