Table 5: Derived masses and ages using the Baraffe et al. (1998) evolutionary tracks

Object
A_V Mass ( $M_\odot$ ) Age (Myr)

Sz100 0 0.2 $\sim$ 1.5

Sz106 3.3 0.45 18

Sz108A 0 0.5 $\sim$ 1.5

Sz108B 0 0.1 $\sim$ 1.5

Sz109 0 0.08 $\sim$ 1

Sz110 2.2 0.25 $\sim$ 1.5

Sz112 0 0.12 $\sim$ 1

Sz113 0.1 0.09 3

Sz114 0.5 0.15 $\sim$ 1

Par-Lup3-1 0 0.04 $\sim$ 1

Par-Lup3-2 0 0.11 $\sim$ 1

Par-Lup3-3 4.3 0.3 $\sim$ 1

Par-Lup3-4 5.6 - 2.4¹ 0.12 50

Note:

¹ The two values of the extinction given correspond respectively

to the photometry given in this paper (July 2002) and to that

published by Nakajima et al. (2000).

**Table 5:** Derived masses and ages using the Baraffe et al. (1998) evolutionary tracks
Object	A_V	Mass ( $M_\odot$ )	Age (Myr)
Sz100	0	0.2	$\sim$ 1.5
Sz106	3.3	0.45	18
Sz108A	0	0.5	$\sim$ 1.5
Sz108B	0	0.1	$\sim$ 1.5
Sz109	0	0.08	$\sim$ 1
Sz110	2.2	0.25	$\sim$ 1.5
Sz112	0	0.12	$\sim$ 1
Sz113	0.1	0.09	3
Sz114	0.5	0.15	$\sim$ 1
Par-Lup3-1	0	0.04	$\sim$ 1
Par-Lup3-2	0	0.11	$\sim$ 1
Par-Lup3-3	4.3	0.3	$\sim$ 1
Par-Lup3-4	5.6 - 2.4¹	0.12	50

Source LaTeX | All tables | In the text

Note:
¹ The two values of the extinction given correspond respectively
to the photometry given in this paper (July 2002) and to that
published by Nakajima et al. (2000).