Table 15: Sample stars with Li upper limits. The stars with a * lie in the ranges in effective temperature and metallicity chosen to delimitate the Li plateau. The others are either cooler or more metal-rich. The $\char93$ indicates the stars for which a v sin i value higher than 4.5 km s^-1 could be derived by Ryan et al. (2002) or Ryan & Elliott (2004). See the text for more details.

HIP ${T}_{\rm eff}$ Log $L/L_{\odot}$ [Fe/H] Li u.l. single

/binary

Dwarfs

72561 ^* $\char93$ 6388 $-0.12\pm0.30$ -1.66 1.639 b

100682 ^* $\char93$ 6362 $-0.12\pm0.20$ -2.83 1.088 b

67655 5429 $-0.38\pm0.04$ -1.03 1.245 s

67863 5683 $-0.04\pm0.04$ -0.88 1.338 s

Subgiants

81276 ^* $\char93$ 6523 $0.76\pm0.58$ -1.50 1.705 b

83320 ^* $\char93$ 5984 $0.71\pm0.77$ -2.56 1.265 s

55022 $\char93$ 6367 $0.50\pm0.14$ -1.29 1.313 s

60719 5319 $1.44\pm0.21$ -2.32 0.789 s

**Table 15:** Sample stars with Li upper limits. The stars with a * lie in the ranges in effective temperature and metallicity chosen to delimitate the Li plateau. The others are either cooler or more metal-rich. The $\char93$ indicates the stars for which a v sin i value higher than 4.5 km s^-1 could be derived by Ryan et al. (2002) or Ryan & Elliott (2004). See the text for more details.
HIP			${T}_{\rm eff}$	Log $L/L_{\odot}$	[Fe/H]	Li u.l.	single
							/binary
Dwarfs
72561	^*	$\char93$	6388	$-0.12\pm0.30$	-1.66	1.639	b
100682	^*	$\char93$	6362	$-0.12\pm0.20$	-2.83	1.088	b
67655			5429	$-0.38\pm0.04$	-1.03	1.245	s
67863			5683	$-0.04\pm0.04$	-0.88	1.338	s
Subgiants
81276	^*	$\char93$	6523	$0.76\pm0.58$	-1.50	1.705	b
83320	^*	$\char93$	5984	$0.71\pm0.77$	-2.56	1.265	s
55022		$\char93$	6367	$0.50\pm0.14$	-1.29	1.313	s
60719			5319	$1.44\pm0.21$	-2.32	0.789	s

Source LaTeX | All tables | In the text

	1 The lithium paradigm
	2 The "Lithium plateau debate''?
	3 Sample selection: a critical analysis of the literature
	4 Stellar parameters: I. Gravity, metallicity, and microturbulence
	5 Stellar parameters. II. The temperature scale and its weaknesses
	6 Our final choice: temperature and data-sample(s)
	7 The lithium abundance
	8 Preliminary results on the mean lithium abundance and the dispersion
	9 Evolutionary status of the stars
	10 The lithium abundance along the plateau for the dwarf stars
	11 The lithium abundance in evolved stars
	12 Duplicity and variability
	13 Stars with extreme Li abundances
	14 Implications for stellar structure and evolution
	15 Summary and conclusions
	References
	Online Material