Table 4: Abundance of iron and of some elements determined in the present work. The columns provide, respectively, the atomic number, the element symbol, the number of lines analyzed, the mean abundance in the atmosphere of HD 221170 with respect to solar photosphere (Grevesse & Sauval 1998) and the abundance in the scale log N(H) = 12.
Z Ident. N $\Delta$ log N log N

26 Fe I 221 -2.09+0.07 5.41 $\pm$ 0.07

Fe II 30 -2.09+0.17 5.41 $\pm$ 0.17

63 Eu II 6 -1.54+0.13 -1.03 $\pm$ 0.13

76 Os I 4 -1.23+0.12 0.22 $\pm$ 0.12

77 Ir I 1 0.17 $\pm$ 0.20

82 Pb I 1 -1.85+0.20 0.10 $\pm$ 0.20

90 Th II 5 -1.18 $\pm$ 0.11

92 U II 5 <-2.02 $\pm$ 0.20

**Table 4:** Abundance of iron and of some elements determined in the present work. The columns provide, respectively, the atomic number, the element symbol, the number of lines analyzed, the mean abundance in the atmosphere of HD 221170 with respect to solar photosphere (Grevesse & Sauval 1998) and the abundance in the scale log N(H) = 12.
Z	Ident.	N	$\Delta$ log N	log N
26	Fe I	221	-2.09+0.07	5.41 $\pm$ 0.07
	Fe II	30	-2.09+0.17	5.41 $\pm$ 0.17
63	Eu II	6	-1.54+0.13	-1.03 $\pm$ 0.13
76	Os I	4	-1.23+0.12	0.22 $\pm$ 0.12
77	Ir I	1		0.17 $\pm$ 0.20
82	Pb I	1	-1.85+0.20	0.10 $\pm$ 0.20
90	Th II	5		-1.18 $\pm$ 0.11
92	U II	5		<-2.02 $\pm$ 0.20

Source LaTeX | All tables | In the text

	1 Introduction
	2 Observations and atmospheric parameters
	3 Abundance analysis
	4 Discussion
	5 Conclusion
	References
	Online Material