**Table 2:** Stars classified as metal-deficient barium stars by Mennessier et al. (1997). The absolute magnitude M_V is a maximum likelihood estimate obtained by Mennessier et al. (1997), except for the additional stars where it is derived from a straight inversion of the Hipparcos parallax (BD $+75^\circ 348$ ), from a spectroscopic estimate of gravity and an educated guess for the mass (BD + $3^\circ 2688$ ) or from a fit to the M 92 isochrone (CS stars). The column labelled "Ba'' indicates whether detailed chemical analyses have confirmed the Ba nature of the star.
HIP	HD/DM	M_V	B-V	[Fe/H]	Ref.	Ba	Ref.	Rem.
4347	5424	-0.6	1.14
11595	15589	-0.5	1.15	-0.7	9
25161	$-27^\circ$ 2233	-1.1	1.13
29740	43389	-3.5	1.48
34795	55496	-1.7	0.96	-1.55	5	y	5
58596	104340	-1.9	1.36	-1.72	3	y	3
69834	123396	-0.9	1.19
76605	139409	-0.5	1.04	-0.42	2	mild	2	M_V = 1.5 is derived from spectroscopic $\log g$
80843	148897	-1.8	1.27	-1.0	2	n	2
				-0.62	7
				-1.16	8
97874	187762	-1.2	1.10
107478	206983	0.2	1.64	-1.43	3	y	3
Additional stars (from refs. (1), (5) and (10))
43042	+ $75^\circ 348$	-0.4:	1.17	-0.8	1	y	1
55852	+ $4^\circ 2466$	?	0.60	-1.85	5,11	y	4, 5
	+ $3^\circ 2688$	-5.0	1.22	-1.42	5,11	y	5
	CS 22942-019	0	0.74	-2.67	10	y	10
	CS 22948-027	-1	0.93	-2.60	10	y	10

References to the table: (1) Zacs et al. (2000); (2) this work; (3) Junqueira & Pereira (2001); (4) Burris et al. (2000); (5) Luck & Bond (1991); (6) Jorissen et al. (1998); (7) Kyröläinen et al. (1986); (8) Luck (1991); (9) Barbuy et al. (1992); (10) Preston & Sneden (2001); (11) B-V from the Tycho-2 catalog (Høg et al. 2000b).

Source LaTeX | All tables | In the text