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Table 4

Abundances and depletions.

Source δX AX AXA
(1017 cm−2) (10−5 H−1) (10−5 H−1)
Magnesium

GRS 1758-258 7.7 ± 0.5 >0.97 3.6 ± 0.3 3.6 ± 0.3 0.9 ± 0.1
GRS 1915+105 20 ± 3 0.8 ± 0.1 4.0 ± 0.5 3.0 ± 0.2 1.0 ± 0.1
GX 17+2 9.4 ± 2.2 >0.97 4.3 ± 0.9 4.3 ± 0.9 1.0 ± 0.3
GX 3+1 7.0 ± 0.1 >0.99 3.7 ± 0.1 3.7 ± 0.1 0.9 ± 0.1
GX 9+1 8.5 ± 3.5 >0.90 5 ± 2 5 ± 2 1.3 ± 0.5
H1743-322 9.6 ± 2.8 >0.74 4 ± 1 3.0 ± 0.7 0.9 ± 0.3
IGR J17091-3624 4.4 ± 0.2 >0.96 3.6 ± 0.2 3.6 ± 0.2 0.9 ± 0.1
LMC X-1 1.4 ± 0.3 >0.99 0.8 ± 0.2 0.7 ± 0.2 0.20 ± 0.05

Silicon

GRS 1758-258 8.4 ± 0.8 0.98 ± 0.01 3.9 ± 0.4 3.8 ± 0.4 1.0 ± 0.1
GRS 1915+105 22 ± 2 0.98 ± 0.01 4.2 ± 0.3 4.2 ± 0.3 1.1 ± 0.1
GX 17+2 9.3 ± 2.0 0.98 ± 0.01 4.3 ± 0.9 4.2 ± 0.9 1.1 ± 0.2
GX 3+1 8.7 ± 0.2 0.96 ± 0.01 4.5 ± 0.1 4.4 ± 0.1 1.2 ± 0.1
GX 9+1 7.7 ± 2.3 0.96 ± 0.03 5 ± 1 5 ± 1 1.2 ± 0.4
H1743-322 11 ± 3 0.97 ± 0.02 4 ± 1 4 ± 1 1.0 ± 0.3
IGR J17091-3624 4.8 ± 0.3 0.98 ± 0.01 4.0 ± 0.3 3.9 ± 0.3 1.0 ± 0.1
LMC X-1 0.9 ± 0.3 >0.98 0.5 ± 0.1 0.5 ± 0.1 0.13 ± 0.04

Notes. The parameter represents the total column density of the X element, δX its depletion from the gas phase, AX the total abundance, and the abundance of the X element in dust. In Sect. 4.4 we provide for LMC X-1 the abundance ratios obtained assuming the Large Magellanic Cloud abundances listed in Table A.2.

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