VizieR

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

VizieR

  
J/AJ/145/167
  Abundances of LX Per (Kang+, 2013)
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2013AJ....145..167K
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Post annotation 		  
1.J/AJ/145/167/table1Iron lines in the spectrum of LX Per (107 rows)
2.J/AJ/145/167/linesLines of non-iron elements in the spectrum of LX Per (tables 5 and 6) (233 rows)
3.J/AJ/145/167/table7Mean abundances of chemical elements in the atmosphere of LX Per (53 rows)
4.J/AJ/145/167/refsReferences (15 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)M (char) Mean abundance for this element (meta.ref.url)
  (1+2+3)Ion (char) Iron line identifier (Fe I or Fe II) (phys.atmol.ionStage)
  (1+2)lambda 0.1nm [4515/8946] Wavelength; in Å (em.wl)
  (1+2)loggf [-] Log of the oscillator strength (phys.atmol.oscStrength)
   (1+2)r_loggf (char) Reference for loggf; in refs.dat file (meta.ref;pos.frame)
  (1+2)Elow eV Lower excitation energy level (phys.energy;phys.atmol.level)
  (1)EWh 0.1pm (n) Equivalent width of hot component (mÅ) (spect.line.eqWidth)
  (1)EWc 0.1pm (n) Equivalent width of cool component (mÅ) (spect.line.eqWidth)
  (1)logNh [-] (n) Hot component abundance (logN(H)=12) (phys.abund)
  (1)logNc [-] (n) Cool component abundance (logN(H)=12) (phys.abund)

ALL cols		    
(n) indicates a possible blank or NULL column(i)indexed column
  (2+3)C (char) hotter (table5) or cooler (table6) component (meta.code.multip)
  (2)f_loggf (char) [h] Flag on loggf (h) (Note 1)   (meta.code)
  (2)logN [-] Derived abundance in LX Per (H=12) (phys.abund)
  (2)logNo [-] (n) Derived abundance in the Sun (H=12) (phys.abund)
  (2)Abun [Sun] LX Per abundance relative to the Sun (phys.abund)
  (2)Bl   [0/1] Blending in LX Per (1=clean line) (meta.note)
  (2)Blo  (n) [0/1] Blending in the Sun (1=clean line) (meta.note)
  (2)D   [0/1] LX Per depth in synthetic spectrum (phot.flux.density;arith.ratio)
  (2)Do  (n) [0/1] Solar depth in synthetic spectrum (phot.flux.density;arith.ratio)
  (2)e(g) [-] LX Per error in abundance for a change in logg of +0.2dex (stat.error)
  (2)e(T) [-] LX Per error in abundance for a change in effective temperature of +100K (stat.error)
  (3)Z  (n) [3/56] Atomic number (meta.id;meta.main)
  (3)NL   [1/72] Number of spectral lines used (meta.number)

ALL cols		    
(n) indicates a possible blank or NULL column(i)indexed column
  (3)Lines (char) Details of lines observed for this element (meta.ref.url)
  (3)Abest [Sun] Best value mean abundance (LX Per minus Solar) (phys.abund)
  (3)e_Abest [Sun] (n) Uncertainty in Ab-best (stat.error)
  (3)Ag+0.2 [Sun] Mean abundance (LX Per minus Solar) with surface gravity shifted by +0.2cm/s2 (phys.abund)
  (3)e_Ag+0.2 [Sun] (n) Uncertainty in Ag+0.2 (stat.error)
  (3)A+100K [Sun] Mean abundance (LX Per minus Solar) with effective temperature altered by +100K (phys.abund)
  (3)e_A+100K [Sun] (n) Uncertainty in A+100K (stat.error)
  (3)Nbest [-] Best value of LX Per absolute mean abundance log(N/H)+12 (phys.abund)
  (3)e_Nbest [-] (n) Uncertainty in N-best (stat.error)
  (3)Ng+0.2 [-] Absolute mean abundance of LX Per with surface gravity shifted by +0.2cm/s2 (phys.abund)
  (3)e_Ng+0.2 [-] (n) Uncertainty in N+0.2 (stat.error)
  (3)N+100K [-] Absolute mean abundance (log(N/H)+12) of LX Per with effective temperature altered by +100K (phys.abund)
  (3)e_N+100K [-] (n) Uncertainty in N+100K (stat.error)

ALL cols		    
(n) indicates a possible blank or NULL column(i)indexed column
  (4)Ref   [1/27] Reference number (meta.id;meta.main)
  (4)BibCode (char) Bibliographic code (meta.bib.bibcode)
  (4)Aut (char) Authors's name (meta.bib.author)
  (4)Com (char) Comments (meta.note)

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