Table 7: Physical parameters for the two components of the $\varepsilon$ Indi Ba,Bb system derived using the COND models of Baraffe et al. (2003) covering the plausible range of ages (0.8, 1.3, and 2.0 Gyr) for the system (Lachaume et al. 1999; SMLK03). See text for a detailed discussion of the derivation and the errors in the assumptions, as well as the masses derived in similar fashion from the Burrows et al. (1997) models.
Source M_K BC_K $M_{\rm bol}$ $\log L/\mbox{~$L_{\odot}$\/}$ Mass Radius $T_{\rm eff}$

$M_{\rm Jup}$ $R/\mbox{~$R_{\odot}$\/}$ K

0.8 1.3 2.0 0.8 1.3 2.0 0.8 1.3 2.0

$\varepsilon$ Indi Ba $13\hbox{$.\!\!^{\rm m}$ }58$ $2\hbox{$.\!\!^{\rm m}$ }88$ $16\hbox{$.\!\!^{\rm m}$ }46$ -4.71 38 47 57 0.096 0.091 0.086 1238 1276 1312

$\varepsilon$ Indi Bb $15\hbox{$.\!\!^{\rm m}$ }85$ $2\hbox{$.\!\!^{\rm m}$ }22$ $18\hbox{$.\!\!^{\rm m}$ }07$ -5.35 22 28 35 0.101 0.096 0.092 835 854 875

**Table 7:** Physical parameters for the two components of the $\varepsilon$ Indi Ba,Bb system derived using the COND models of Baraffe et al. (2003) covering the plausible range of ages (0.8, 1.3, and 2.0 Gyr) for the system (Lachaume et al. 1999; SMLK03). See text for a detailed discussion of the derivation and the errors in the assumptions, as well as the masses derived in similar fashion from the Burrows et al. (1997) models.
Source	M_K	BC_K	$M_{\rm bol}$	$\log L/\mbox{~$L_{\odot}$\/}$	Mass	Radius	$T_{\rm eff}$
					$M_{\rm Jup}$	$R/\mbox{~$R_{\odot}$\/}$	K
					0.8	1.3	2.0	0.8	1.3	2.0	0.8	1.3	2.0
$\varepsilon$ Indi Ba	$13\hbox{$.\!\!^{\rm m}$ }58$	$2\hbox{$.\!\!^{\rm m}$ }88$	$16\hbox{$.\!\!^{\rm m}$ }46$	-4.71	38	47	57	0.096	0.091	0.086	1238	1276	1312
$\varepsilon$ Indi Bb	$15\hbox{$.\!\!^{\rm m}$ }85$	$2\hbox{$.\!\!^{\rm m}$ }22$	$18\hbox{$.\!\!^{\rm m}$ }07$	-5.35	22	28	35	0.101	0.096	0.092	835	854	875

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