Chemical abundances for the outer halo cluster Pal 4 from co-added high-resolution spectroscopy

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Table 5:

Pal 4 abundances relative to comparison clusters.
Name	[Fe/H]	$R_{\rm GC}$ [kpc]	N	$\langle\Delta$ [X/Fe] $\rangle_{\rm all}$	$\langle\Delta$ [X/Fe] $\rangle_{Z<39}$	$\langle\Delta$ [X/Fe]/ ${\sigma}{\rangle}_{\rm all}$	$\langle\Delta$ [X/Fe]/ ${\sigma}{\rangle}_{Z<39}$	Reference^a
(1)	(2)	(3)	(4)	(5)	(6)	(7)	(8)	(9)
NGC 6752	-1.61	5.2	17	0.18 $\pm$ 0.06	0.10 $\pm$ 0.08	1.0	0.5	(1), (2)
M 13	-1.56	8.7	17	0.15 $\pm$ 0.06	0.04 $\pm$ 0.06	0.8	0.2	(1), (3)
M 3	-1.39	12.3	18	0.09 $\pm$ 0.06	-0.01 $\pm$ 0.08	0.5	0.0	(1), (3)
NGC 7492	-1.87	24.9	16	0.09 $\pm$ 0.05	0.02 $\pm$ 0.05	0.4	0.1	(1), (4)
NGC 5694	-2.06	29.1	10	0.36 $\pm$ 0.12	0.14 $\pm$ 0.06	1.8	0.6	(1), (5)
Pal 3	-1.58	95.9	19	0.05 $\pm$ 0.05	-0.05 $\pm$ 0.06	0.3	-0.1	(1), (6)

Notes. ^(a) (1) Web-version (2003) of Harris (1996); (2) Yong et al. (2005); (3) Cohen & Meléndez (2005b); (4) Cohen & Meléndez (2005a); (5) Lee et al. (2006); (6) Paper I.

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