Table 3: Abundance ratios [X/Fe] for varying collision parameter $S_{\!\!\rm H}$ compared with LTE results for a typical turnoff star, where X represents the elements Na, Mg and Al. All abundance ratios refer to abundances calculated for the spectra of G165-39.
Ion Line $S_{\!\!\rm H}= 0.001$ 0.01 0.1 1.0 LTE

Na I 5889 Å -0.44 -0.44 -0.43 -0.33 0.04

Mg I 5184 Å 0.06 0.06 0.07 0.07 0.07

Al I 3961 Å -0.21 -0.21 -0.21 -0.26 -1.05

**Table 3:** Abundance ratios [X/Fe] for varying collision parameter $S_{\!\!\rm H}$ compared with LTE results for a typical turnoff star, where X represents the elements Na, Mg and Al. All abundance ratios refer to abundances calculated for the spectra of G165-39.
Ion	Line	$S_{\!\!\rm H}= 0.001$	0.01	0.1	1.0	LTE
Na I	5889 Å	-0.44	-0.44	-0.43	-0.33	0.04
Mg I	5184 Å	0.06	0.06	0.07	0.07	0.07
Al I	3961 Å	-0.21	-0.21	-0.21	-0.26	-1.05

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