Astronomy & Astrophysics

Table 3: Properties of the Clusters, the age is derived from the EW of $\rm H\alpha$ , A_V from the Balmer decrement.
M_V EQW( $\rm H\alpha$ ) Age (Myr) A_V M( $10^5 ~M_{\odot}$ )

1 -13.28 $730\pm20$ 4.7 0.77 7.2

2 -12.15 $325\pm20$ 5.1 0.49 1.2

3 -12.82 $230\pm10$ 5.8 0.11 2.1

4 -11.54 - - - -

5 -11.67 $33\pm 5$ 10.0 - 2.9

6 -11.93 $260\pm10$ 5.6 0.77 1.6

7 -11.57 - - - -

8 -11.36 - - - -

**Table 3:** Properties of the Clusters, the age is derived from the EW of $\rm H\alpha$ , A_V from the Balmer decrement.
	M_V	EQW( $\rm H\alpha$ )	Age (Myr)	A_V	M( $10^5 ~M_{\odot}$ )
1	-13.28	$730\pm20$	4.7	0.77	7.2
2	-12.15	$325\pm20$	5.1	0.49	1.2
3	-12.82	$230\pm10$	5.8	0.11	2.1
4	-11.54	-	-	-	-
5	-11.67	$33\pm 5$	10.0	-	2.9
6	-11.93	$260\pm10$	5.6	0.77	1.6
7	-11.57	-	-	-	-
8	-11.36	-	-	-	-

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