Table 3: Elemental abundances in HR 5049. Consecutive columns are as follows: the name of ion, the number of used lines, the derived abundance, the standard deviation, the solar log $\epsilon $, and the logarithmic abundance for HR 5049 relative to the Sun.

Ions		 n log $\epsilon $ S.D. log $\epsilon $$\odot$ $\Delta$log $\epsilon $

He I		   $\le$9.0   10.99 $\le$-2.0
C II   $\le$8.3   8.55 $\le$-0.25
O I   8.31   8.87 -0.56
Mg I 2 7.30 0.42 7.84 -0.54
Mg II 4 7.15 0.19   -0.69
Si II 3 7.75 0.09 7.55 +0.20
Cl II 3 7.39 0.17 5.5 +1.9
Sc II 1 3.06   3.17 -0.11
Ti II 6 5.49 0.38 5.02 +0.47
V II 1 4.75   4.00 +0.75
Cr I 4 7.61 0.45 5.67 +1.94
Cr II 18 7.36 0.48   +1.69
Mn II 3 6.30 0.00 5.39 +0.91
Fe I 10 8.32 0.17 7.50 +0.82
Fe II 35 8.29 0.32   +0.79
Co I 7 8.43 0.08 4.92 +3.51
Co II 12 8.35 0.37   +3.43
Ni II 1 6.90   6.25 +0.65
Sr II 2 2.96 0.16 2.97 -0.01
Y II 4 4.33 0.37 2.24 +2.09
Ba II 1 $\le$2.1   2.13 $\le$0.0
La II 1 4.00   1.17 +2.83
Ce II 4 4.68 0.21 1.58 +3.10
Pr II 1 4.70   0.71 +3.99
Pr III 10 4.68 0.27   +3.97
Nd III 3 4.74 0.13 1.50 +3.24
Eu II 2 4.06 0.42 0.51 +3.55
Eu III 2 5.30 0.42 0.51 +4.79
Gd II 5 4.53 0.28 1.12 +3.41
Dy II 1 4.75   1.14 +3.61
Dy III 1 4.07   1.14 +2.93


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