Table 4: Abundances for HD 139409, in the scale where (H) = 12, and normalized with respect to the solar abundances (Grevesse & Sauval 1998). The standard deviations  and the number N of lines used in the analysis are also given.

Element(X)	Z	(X)		N	[X/Fe]
C  I	6	8.46	0.10	4	+0.36
Na  I	11	6.02	0.05	5	+0.11
Mg  I	12	7.31	0.12	6	+0.15
Si  I	14	7.33	0.06	20	+0.20
Ca  I	20	6.20	0.07	6	+0.26
Sc  II	21	2.79	0.06	10	+0.04
Ti  I	22	4.77	0.09	51	+0.17
Ti  II	22	4.72	0.11	4	+0.12
V  I	23	3.76	0.11	23	+0.18
Cr  I	24	5.21	0.11	11	-0.04
Cr  II	24	5.36	0.09	3	+0.11
Mn  I	25	5.13	0.11	9	+0.16
Fe  I	26	7.08	0.08	136	-
Fe  II	26	7.08	0.12	14	-
Ni  I	28	5.86	0.07	44	+0.03
Y  I	39	2.22	0.10	2	+0.40
Y  II	39	2.41	0.07	6	+0.59
Zr  I	40	2.58	0.09	3	+0.40
Zr  II	40	2.78	0.12	3	+0.60
Ba  II	56	1.89	0.12	3	+0.18
La  II	57	1.05	0.12	3	+0.30
Ce  II	58	1.46	0.14	5	+0.30
Nd  II	60	1.38	0.09	6	+0.30