VizieR

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

VizieR

  
J/AJ/149/59
  Abundances of ρ Pup (Yushchenko+, 2015)
Post annotation
  
1.J/AJ/149/59/table1Iron lines in the spectrum of ρ Pup (167 rows)
2.J/AJ/149/59/table2Abundances of chemical elements in the atmosphere of ρ Pup: individual lines (430 rows)
3.J/AJ/149/59/table3Abundances of chemical elements in the atmosphere of ρ Pup: mean values (73 rows)

 
Query by Constraints constraints help applied on Columns (Output Order: + - )
ShowSortJoin tables
more join
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)
   (ALL)Ion (char) Iron line identifier (Fe I or Fe II) (phys.atmol.ionStage)
  (1+2)lambda 0.1nm [4620/8839] Wavelength λ; in Å (em.wl)
  (1+2)loggf [-] [-5.24/0.53] Log of the oscillator strength (phys.atmol.oscStrength)
  (1+2)r_loggf  Reference for loggf (Note G2)   (meta.ref;phys.atmol)
  (1+2)Elow eV [0/10.48] Lower level energy (phys.energy;phys.atmol.level)
  (1)EW 0.1pm [4/198] Equivalent width; in mÅ (spect.line.eqWidth)
  (1)logN [-] [7.783/8.03] Log number abundance (Note G3)   (phys.abund)
  (2+3)Tel (char) Telescope facility used (IUE or VLT) (Note G1)   (meta;instr.setup)
  (2)logN* [-] Log number absolute abundance in ρ Pup (Note G3)   (phys.abund)

ALL cols
    
 (i)indexed column
  (2)logNo [Sun] (n) Log number absolute abundance in the Sun (Note G3)   (phys.abund)
  (2)Abund [Sun] Difference between logN* and logNS (Note 1)   (phys.abund;arith.diff)
  (2)Inp*  Relative input of the investigated line to the line absorption coefficient in synthetic spectrum of ρ Pup (1=Clean line, 0=Very weak line) (Note 2)   (meta.note)
  (2)Inpo  (n) Relative input of the investigated line to the line absorption coefficient in synthetic spectrum of the Sun (1=Clean line, 0=Very weak line) (Note 2)   (meta.note)
  (2)Depth*  Depth of line in synthetic spectrum of ρ Pup (phys.absorption.opticalDepth)
  (2)Deptho  (n) Depth of line in synthetic spectrum of the Sun (phys.absorption.opticalDepth)
  (2)d(T) [-] (n) Change in logN* for Teff=+100K (Note 3)   (phys.abund)
  (2)d(g) [-] (n) Change in logN* for logg=-0.3 (Note 3)   (phys.abund)
  (3)Z   [3/90] Atomic number (meta.id;meta.main)
  (3)Nl   [1/120] Number of lines used (phys.abund)
  (3)Abest [Sun] Best value mean abundance (ρ Pup minus Solar) (Note 1)   (phys.abund)
  (3)e_Abest [Sun] (n) 1σ uncertainty in Abest (stat.error)
  (3)A+100K [Sun] Mean abundance (ρ Pup minus Solar) with effective temperature increased by +100K (phys.abund)

ALL cols
    
(n) indicates a possible blank or NULL column(i)indexed column
  (3)e_A+100K [Sun] (n) 1σ uncertainty in A+100K (stat.error)
  (3)Ag+0.2 [Sun] Mean abundance (ρ Pup minus Solar) with surface gravity decreased by +0.2cm/s2 (phys.abund)
  (3)e_Ag+0.2 [Sun] (n) 1σ uncertainty in Ag+0.2 (stat.error)
  (3)Nbest [-] Best value of ρ Pup absolute mean abundance (Note 2)   (phys.abund)
  (3)e_Nbest [-] (n) 1σ uncertainty in Nbest (stat.error)
  (3)N+100K [-] Absolute mean abundance of ρ Pup with effective temperature increased by +100K (phys.abund)
  (3)e_N+100K [-] (n) 1σ uncertainty in N+100K (stat.error)
  (3)Ng+0.2 [-] Absolute mean abundance of ρ Pup with surface gravity decreased by +0.2cm/s2 (phys.abund)
  (3)e_Ng+0.2 [-] (n) 1σ uncertainty in Ng+0.2 (stat.error)

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

Thanks for acknowledging the VizieR Service
Rules of usage of VizieR data

© Université de Strasbourg/CNRS

    • Contact