Table 2: Equivalent widths of the main emission lines observed in the spectra of the stars discussed in this paper.

Object	[OI]	[OI]	H	[NII]	HeI	[SII]	[SII]	[OII]	[OII]	OI	CaII	CaII	CaII
	6300	6364	6563	6583	6678	6716	6731	7319	7329	8446	8498	8542	8662
Sz100			(84)						-	-	5.4	5.0	4.3
Sz102	157	50.5	445	44	4:	19	43	70.4		7.3	24.9	31	25
Sz106	3.3	0.7	110		1.5	0.9		-	-	0.8	1.0	0.2:	0.6:
Sz108A						-	-	-	-	-	-	-	-
Sz108B	1.6	-	53		-	-	-	-	-	-	-	-	-
Sz109	-	-	15		-	-	-	-	-	-	-	-	-
Sz110	-	-	42		2.2	-	-	-	-	-	-	-	-
Sz112	-	-	23.5			-	-	-	-	-	-	-	-
Sz113	-	-	139		2.6	-	-	-	-	-	8.0	8.0	6.0
Sz114			(24)					-	-	-	-	-
Par-Lup3-1	-	-	12		-	-	-	-	-	-	-	-	-
Par-Lup3-2			(6.5)					-	-	-	-	-
Par-Lup3-3			19		-	-	-	-	-	-	-	-	-
Par-Lup3-4	133	42	410	9:	1.6	21	38	3:		5.5	14.5	13.8	10.0
LS-RCrA 1	92	25	360	15	1.5	12.4	19.2	3.6	3.6		4.0	3.6	2.2

Notes:

H in parentheses are those measured on the slitless spectra.

The symbol "-'' indicates that the line is not detectable, while a blank entry means that the line falls outside the spectral

range covered for that object.