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J/A+A/516/A46/table8 HE 2327-5642 abundance analysis (Mashonkina+, 2010)
Line data and abundances from an analysis of HE 2327-5642 (290 rows)
Post annotation about this record
ColumnValue  Explain   (UCD)
68recno 68  Record number assigned by the VizieR team. Should Not be used for identification. (meta.record)

Z24  Atomic number (;meta.main)
ElCr I  Atom/molecule (phys.atmol.ionStage)
lambda4274.80 0.1nm Wavelength (em.wl)
lambda2  0.1nm Second wavelength when interval (em.wl)
Eexc  eV Excitation energy (phys.atmol.excitation)
loggf-0.230 [-] Adopted gf-value (phys.absorption.coeff)
r_loggfMFW88  Reference for loggf, in refs.dat file (meta.ref;pos.frame)
epsSun 5.64 [-] Solar photosphere abundance (ε(H)=12) (phys.abund)
epsLTE 2.16 [-] LTE abundance (ε(H)=12) (phys.abund)
epsNLTE  [-] NLTE abundance (1)(ε(H)=12) (phys.abund)
[X/Fe]-0.70 [-] Abundance relative to iron (phys.abund)
EW73.9 0.1pm Equivalent width (mÅ) (spect.line.eqWidth)
n_EW    [Syn ] from synthetic spectrum (meta.note)
G6/NH-7.675 [rad/s/cm3] van der Waals damping constant log(Γ6/NH) at 10000K. (arith.zp)
Model1G6  Model used (Note 3)   (;
r_Model1ABO  Reference for Model1, in refs.dat file (meta.ref;pos.frame)
Model2   Model used (Note 3)   (;
r_Model2   Reference for Model2, in refs.dat file (meta.ref;pos.frame)
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