Table 3: Physical characteristics of 2M1207 A and b according to DUSTY models of Chabrier et al. (2000) and Baraffe et al. (2002).
Name Age Mass $T_{\rm {eff}}$ Luminosity Radius

(Myr) ( $M_{\rm {Jup}}$ ) (K) log( $L/L_{\odot}$ ) ( $R/R_{\odot})$

2M1207 A 5 25 2600 -2.43 0.31

10 45 2800 -2.36 0.28

2M1207 b 5 4 1163 -4.28 0.15

10 6 1320 -4.24 0.15

**Table 3:** Physical characteristics of 2M1207 A and b according to DUSTY models of Chabrier et al. (2000) and Baraffe et al. (2002).
Name	Age	Mass	$T_{\rm {eff}}$	Luminosity	Radius
	(Myr)	( $M_{\rm {Jup}}$ )	(K)	log( $L/L_{\odot}$ )	( $R/R_{\odot})$
2M1207 A	5	25	2600	-2.43	0.31
	10	45	2800	-2.36	0.28
2M1207 b	5	4	1163	-4.28	0.15
	10	6	1320	-4.24	0.15

Source LaTeX | All tables | In the text

	1 Introduction
	2 Observations
	3 Companionship confirmation
	4 Discussion
	5 Conclusion
	References