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Table 6:

Table of elements and spectral lines used for mapping of HD 50773.
Species $\lambda$ (Å) $\log gf$ $E_{\rm low}$ (eV) min, max Blended with $\odot$
        $\log(N/N_{{\rm tot}})$   $\log(N/N_{{\rm tot}})$
Mg   I 5401.5210 -0.340 11.6300   Fe, Y -4.51
Si   II 5055.9840 0.593 10.0740 -4.8, -2.6   -4.53
Si   I 5421.1680 -2.250 5.6190   Cr, Mn  
Si   I 5421.3830 -1.480 5.6190   Cr, Mn  
Ca   I 6102.7230 -0.862 1.8790 -6.5, -2.7 Fe -5.73
Ca   II 6456.8750 -0.539 8.4380   Fe  
Ti   II 5154.0680 -1.750 1.5660 -8.3, -6.1 Cr, Fe -7.14
Cr   II 5237.3290 -1.350 4.0730 -7.1, -3.6   -6.40
  5280.0540 -2.316 4.0740      
  5510.7020 -2.614 3.8270   Fe, Y, Ni  
Fe   I 5383.3692 0.645 4.3120 5.4, -3.6   -4.59
  5400.5022 -0.160 4.3710      
  5400.6560 -2.482 3.6350      
  5401.2689 -1.920 4.3200      
Ni   I 5510.0030 -0.900 3.8470 -6.1, -5.6 Cr, Fe, Y -5.81
Y   II 5509.8950 -1.010 0.9920 -9.9, -7.5 Cr, Fe, Ni -9.83
  5662.9250 0.160 1.9440   Fe  
Cu   II 5153.2300 0.217 3.7860 -8.0, -6.9 Cr, Ti, Fe -7.83

Notes. Element, spectral lines used, the $\log gf$ values of these lines, abundance interval in dex, for comparison the solar values (Asplund et al. 2005) are presented. Atomic parameters used in our study were extracted from VALD.


Source LaTeX | All tables | In the text

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