Table 5: Abundances for HD 137569 compared with other post-AGB and PNe stars.

Star		 $T_{\rm eff}$ [C/H] [N/H] [O/H] [Mg/H] [Si/H] [S/H] [Fe/H]

LS IV $-4\hbox{$.\!\!^\circ$ }01$1		 11 000 <-1.21     -1.98 -2.05    
LS IV $-4\hbox{$.\!\!^\circ$ }01$8 10 000       -2.78 -1.68   -1.71
HD 1375692 12 000 -0.60 +0.20 +0.05 -2.80 -2.40 -0.10 <-3.0
LB 31931 12 900 <-1.91     -2.08 -2.15    
PG 1323-0863 16 000 <-2.25 -0.98 -0.77 -1.71 -1.37    
PG 1704+2223 18 000 -1.40 -0.89 -0.85 -1.37 -1.13    
PHL 1744 18 200 <-2.31 -1.11 -0.85 -1.38 -1.05    
Barnard 295 20 000 -2.164 -0.61 -1.151   -1.255   -2.25
BD +330 26426 20 200 -0.93 -0.56 -0.62 -1.1 -0.9    
LB 32191 21 400 -1.71 -0.31 -1.15 -0.58 -0.95    
ROA 57015 24 000 -2.57 -1.04 -0.78   -1.41   -2.71
LS IV $-12\hbox{$.\!\!^\circ$ }111$1 24 000 -1.71 -0.11 +0.05 -0.28 +0.05 -0.6 -0.41
LS IV $-12\hbox{$.\!\!^\circ$ }111$7 24 000 -0.63 +0.29 +0.05 -0.28 +0.08 -0.5  
References: (1) McCausland et al. (1992), (2) this work, (3) Moehler & Heber (1998), (4) Conlon et al. (1991), (5) Moehler et al. (1998), (6) Napiwotzki et al. (1994), (7) Conlon et al. (1993), (8) Mooney et al. (2002).

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Article Contents
1 Introduction
2 Observations and data reduction
3 Derived elemental abundances
4 Conclusions
References
List of tables
List of figures