Table 10: Abundances for deviating stars. Each star has three columns; abundance; line-to-line scatter (1 $\sigma$ standard deviation); and (in parenthesis) number of lines that were used to derive the abundance.
HIP 2235 HIP 15510 HIP 16788

Thin disk Thick disk Thick disk

$\rm [Fe/H]$ -0.28 0.07 (65) -0.41 0.08 (69) -0.32 0.07 (78)

$\rm [O/H]$ -0.01 0.00 (1) -0.27 0.00 (1)

$\rm [Eu/H]$ -0.19 0.00 (1) -0.06 0.00 (1)

$\rm [Ba/H]$ 0.54 0.06 (4) -0.56 0.08 (3) 0.63 0.06 (4)

$\rm [Y/H]$ 0.31 0.14 (3) 0.09 0.00 (1) 0.45 0.12 (4)

**Table 10:** Abundances for deviating stars. Each star has three columns; abundance; line-to-line scatter (1 $\sigma$ standard deviation); and (in parenthesis) number of lines that were used to derive the abundance.
	HIP 2235	HIP 15510	HIP 16788
	Thin disk	Thick disk	Thick disk
$\rm [Fe/H]$	-0.28	0.07 (65)	-0.41	0.08 (69)	-0.32	0.07 (78)
$\rm [O/H]$			-0.01	0.00 (1)	-0.27	0.00 (1)
$\rm [Eu/H]$	-0.19	0.00 (1)			-0.06	0.00 (1)
$\rm [Ba/H]$	0.54	0.06 (4)	-0.56	0.08 (3)	0.63	0.06 (4)
$\rm [Y/H]$	0.31	0.14 (3)	0.09	0.00 (1)	0.45	0.12 (4)

Source LaTeX | All tables | In the text

	1 Introduction
	2 Stellar sample
	3 Observations and data reductions
	4 Stellar model atmospheres
	5 Abundance analysis
	6 Stellar ages
	7 Abundance results
	8 Discussion and summary
	Appendix A: Kinematical criteria for selecting thick disk stars in the solar neighbourhood
	References