Table 9: Same as Table 7, but for faint stars probably members of either of the two cluster, yet not known to which because of large errors in B-V. For the calculation of bolometric fluxes dependent on apparent magnitude and de-reddened colour, we assumed an average reddening of E(B-V) = 0.05.
X # W # RA DEC $\Delta$ V B-V (B-V)₀ Var log $\frac{L_{\rm x}}{L_{\rm bol}}$

X4 7 42 10 -37 26 47 25 18.23 1.48 1.43 -1.41

X34 7 44 17 -37 47 14 10 18.42 1.50 1.45 -2.41

X35 7 43 13 -37 47 21 25 15.70 1.38 1.33 -2.80

X36 7 44 35 -37 47 28 4 17.62 1.71 1.66 -3.22

X37 7 45 13 -37 47 30 8 17.99 1.65 1.60 -2.83

X38 7 44 49 -37 47 49 1 18.43 1.68 1.63 -2.80

X41 7 44 44 -37 48 08 6 18.06 1.71 1.66 -3.02

X44 7 44 37 -37 49 02 5 16.70 1.47 1.42 -2.78

X49 7 45 33 -37 51 23 3 17.68 1.52 1.47 -2.39

X71 7 44 18 -37 54 17 15 18.62 1.58 1.53 -2.89

X73 7 45 36 -37 54 49 12 16.91 1.59 1.54 -3.25

X76 7 44 37 -37 55 00 3 17.06 1.53 1.48 -3.26

X82 7 45 47 -37 56 19 4 18.75 1.64 1.59 -3.01

X86 7 44 26 -37 56 58 3 18.34 1.52 1.47 -2.38

X87 7 45 10 -37 57 12 2 19.08 1.56 1.51 -2.66

X91 7 46 02 -37 57 47 4 17.47 1.54 1.49 -3.23

X113 7 45 27 -38 00 53 5 18.91 1.61 1.56 -2.84

X121 7 44 36 -38 02 58 2 18.05 1.59 1.54 -3.03

X124 7 43 45 -38 03 56 6 20.25 1.69 1.64 -1.95

X126 7 45 23 -38 04 09 2 19.21 1.94 1.89 -3.24

X130 7 46 02 -38 04 44 15 16.98 1.48 1.43 X -2.78

X136 7 45 29 -38 05 50 2 17.27 1.47 1.42 -2.49

**Table 9:** Same as Table 7, but for faint stars probably members of either of the two cluster, yet not known to which because of large errors in B-V. For the calculation of bolometric fluxes dependent on apparent magnitude and de-reddened colour, we assumed an average reddening of E(B-V) = 0.05.
X #	W #	RA	DEC	$\Delta$	V	B-V	(B-V)₀	Var	log $\frac{L_{\rm x}}{L_{\rm bol}}$
X4		7 42 10	-37 26 47	25	18.23	1.48	1.43		-1.41
X34		7 44 17	-37 47 14	10	18.42	1.50	1.45		-2.41
X35		7 43 13	-37 47 21	25	15.70	1.38	1.33		-2.80
X36		7 44 35	-37 47 28	4	17.62	1.71	1.66		-3.22
X37		7 45 13	-37 47 30	8	17.99	1.65	1.60		-2.83
X38		7 44 49	-37 47 49	1	18.43	1.68	1.63		-2.80
X41		7 44 44	-37 48 08	6	18.06	1.71	1.66		-3.02
X44		7 44 37	-37 49 02	5	16.70	1.47	1.42		-2.78
X49		7 45 33	-37 51 23	3	17.68	1.52	1.47		-2.39
X71		7 44 18	-37 54 17	15	18.62	1.58	1.53		-2.89
X73		7 45 36	-37 54 49	12	16.91	1.59	1.54		-3.25
X76		7 44 37	-37 55 00	3	17.06	1.53	1.48		-3.26
X82		7 45 47	-37 56 19	4	18.75	1.64	1.59		-3.01
X86		7 44 26	-37 56 58	3	18.34	1.52	1.47		-2.38
X87		7 45 10	-37 57 12	2	19.08	1.56	1.51		-2.66
X91		7 46 02	-37 57 47	4	17.47	1.54	1.49		-3.23
X113		7 45 27	-38 00 53	5	18.91	1.61	1.56		-2.84
X121		7 44 36	-38 02 58	2	18.05	1.59	1.54		-3.03
X124		7 43 45	-38 03 56	6	20.25	1.69	1.64		-1.95
X126		7 45 23	-38 04 09	2	19.21	1.94	1.89		-3.24
X130		7 46 02	-38 04 44	15	16.98	1.48	1.43	X	-2.78
X136		7 45 29	-38 05 50	2	17.27	1.47	1.42		-2.49

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