Indi Ba, Bb: a detailed study of the nearest known brown dwarfs

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Table 8:

Physical parameters of $\ensuremath {\varepsilon }$ Indi Ba, Bb derived using the observed luminosities and the COND03 models of Baraffe et al. (2003) for three ages: 1, 5, and 10 Gyr.
Source	log $L/L_{\odot}$	Mass			Radius			$T_{\rm {eff}}$			log g
		( $M_{\rm {Jup}}$ )			( $R_{\odot}$ )			(K)			(cm s^-2)
		1 Gyr	5 Gyr	10 Gyr	1 Gyr	5 Gyr	10 Gyr	1 Gyr	5 Gyr	10 Gyr	1 Gyr	5 Gyr	10 Gyr
$\varepsilon$ Indi Ba	-4.699	42.0	69.8	74.1	0.093	0.080	0.079	1274	1387	1393	5.10	5.45	5.49
$\ensuremath {\varepsilon }$ Indi Bb	-5.232	28.0	57.2	66.2	0.097	0.081	0.077	929	1019	1051	4.88	5.36	5.47

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