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Table 1:

Sample of young clusters in M 33 selected in this work.

ID 		Name RA Dec $12 + \log$(O/H)
    J2000.0  
1 B691 01:34:16.6 30:51:54 $8.26 \pm 0.02$a
2 VGHC 2-84 01:34:06.7 30:48:56 $8.35 \pm 0.04$a
3 IC132 01:33:15.8 30:56:45 $8.08 \pm 0.04$a
4 B290 01:33:11.4 30:45:15 $ 8.21 \pm 0.06$a
5 NGC 588 01:32:45.9 30:38:54 $8.31 \pm 0.06$a
6 C400 01:32:44.4 30:35:17 $7.98 \pm 0.08$b
7 MA2 01:34:15.6 30:37:11 $8.33 \pm 0.08$a
8 S14 01:34:13.7 30:33:45 $8.30 \pm 0.11$b
9 GDK99 128 01:33:59.9 30:32:44 $8.47 \pm 0.06$a
10 C129a 01:33:23.4 30:31:35 $8.45 \pm 0.08$b
11 C121 01:33:17.1 30:31:11 $8.35 \pm 0.06$b
12 B0221 01:33:09.8 30:27:23 $8.28 \pm 0.10$ b
13 B0222 01:33:25.0 30:25:31 $8.10 \pm 0.18$b
14 C022 01:33:01.6 30:24:31 $8.31 \pm 0.08$b
15 B0745 01:34:37.6 30:34:55 $8.07 \pm 0.10$a
16 B0670 01:34:03.3 30:53:09 $8.28 \pm 0.07$a
17 B0637 01:33:50.6 30:56:33 $8.34 \pm 0.05$a
18 LGC HII 3 01:32:45.9 30:41:35 $8.24 \pm 0.05$a
19 B0706 01:34:42.2 30:31:42 $8.32 \pm 0.12$a
20 LGC HII 11 01:34:42.2 30:24:00 $8.17 \pm 0.06$a
21 B0261 01:32:54.6 30:23:22 $8.36 \pm 0.08$b
22 MCM00Em24 01:33:10.8 30:18:08 $8.18 \pm 0.25$a
23 B0254 01:33:21.2 30:17:58 $8.16 \pm 0.19$b
24 LGC HII 2 01:32:43.0 30:19:31 $8.25 \pm 0.06$a
25 B0045 01:33:29.0 30:40:24 $8.49 \pm 0.04$a
26 B0029 01:33:47.8 30:38:38 $8.21 \pm 0.10$b
27 B0016 01:33:50.1 30:37:30 $7.98 \pm 0.19$b
28 B0033b 01:33:34.9 30:37:05 $8.40 \pm 0.08$b
29 B0015b 01:33:50.3 30:33:42 $8.73 \pm 0.23$b
30 B0013c 01:33:54.1 30:33:10 $8.26 \pm 0.12$b
31 B0208f 01:33:34.1 30:32:13 $8.07 \pm 0.06$b
32 C403 01:33:07.6 30:31:01 $8.27 \pm 0.07$b

Notes. The identification names are from: B- Boulesteix et al. (1974); C- Courtes et al. (1987); GDK99- Gordon et al. (1999); LGC-HII-n- Magrini et al. (2007b); VGVC- Viallefond et al. (1986); MCM00- Magrini et al. (2000); MA- Mayall & Aller (1942); S- Searle (1971). Substructure designations within individual cluster (indicated by the letters at the end of their name) are taken from Hodge et al. (2002). The oxygen abundance determinations are from: (a)  Magrini et al. (2007b); (b) Rosolowsky & Simon (2008).


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