Table A.1.
Clusters around GS242-03+37 with ages < 120 Myr.
ID | Name | l (deg) | b (deg) | dhc (kpc) | vLSR (km s−1) | age (Myr) | Δdc–w (kpc) | Y/N | Rem |
---|---|---|---|---|---|---|---|---|---|
1 | NGC 2345 | 226.58 | −2.33 | 2.6 | 40.7 | 79.4 | 0.25 | ||
2 | NGC 2401 | 229.67 | 1.85 | 3.8 | 10.0 | 0.21 | |||
3 | FSR 1228 | 229.88 | −1.61 | 4.2 | 5.6 | 0.40 | |||
4 | NGC 2414 | 231.40 | 1.93 | 2.9 | 47.5 | 18.6 | 0.03 | y | |
5 | DBSB 3 | 231.51 | −4.31 | 3.4 | 10.0 | 0.04 | y | ||
6 | FSR 1243 | 231.98 | 1.99 | 4.3 | 5.0 | 0.35 | |||
7 | DBSB 6 | 234.23 | −0.49 | 4.2 | 3.5 | 0.09 | |||
8 | DBSB 7 | 234.57 | 0.82 | 2.5 | 30.9 | 0.15 | y | ||
9 | DBSB 9 | 234.68 | −0.25 | 4.4 | 1.0 | 0.21 | |||
10 | NGC 2384 | 235.38 | −2.40 | 2.1 | 30.7 | 13.5 | 0.63 | ||
11 | NGC 2421 | 236.27 | 0.07 | 2.2 | 28.2 | 0.52 | |||
12 | DBSB 10 | 237.73 | −0.96 | 2.4 | 3.2 | 0.34 | |||
13 | FSR 1283 | 237.87 | −3.80 | 4.2 | 6.3 | 0.01 | y | ||
14 | Ivanov 6 | 238.48 | −4.29 | 2.4 | 4.0 | 0.27 | |||
15 | FSR 1297 | 239.57 | −4.93 | 3.7 | 5.0 | 0.29 | 1 | ||
16 | Ruprecht 32 | 241.59 | −0.55 | 4.4 | 64.6 | 5.0 | 0.04 | y | |
17 | Haffner 16 | 242.09 | 0.47 | 2.7 | 30.4 | 20.0 | 0.11 | y | |
18 | ESO 429-02 | 242.59 | −4.16 | 2.1 | 7.9 | 0.65 | |||
19 | Haffner 19 | 243.06 | 0.52 | 4.6 | 49.8 | 4.5 | 0.01 | y | |
20 | Trumpler 9 | 243.07 | 1.29 | 2.3 | −34.5 | 63.1 | 0.43 | ||
21 | Haffner 18 | 243.14 | 0.44 | 2.9 | 41.8 | 79.4 | 0.04 | ||
22 | NGC 2467-east | 243.18 | 0.41 | 4.0 | 41.7 | 2.6 | 0.35 | 1 | |
23 | NGC 2453 | 243.27 | −0.94 | 2.4 | 15.5 | 72.4 | 0.35 | ||
24 | Ruprecht 44 | 245.75 | 0.49 | 4.7 | 6.3 | 0.15 | 1 | ||
25 | NGC 2439 | 246.45 | −4.47 | 3.8 | 44.6 | 17.8 | 0.24 | 1 | |
26 | NGC 2489 | 246.72 | −0.77 | 2.3 | 19.7 | 20.9 | 0.58 | ||
27 | Haffner 20 | 246.97 | −0.93 | 2.9 | 114.8 | 0.12 | |||
28 | Haffner 15 | 247.95 | −4.16 | 2.2 | 19.1 | 0.56 | |||
29 | Bochum 15 | 248.00 | −5.48 | 2.4 | 4.7 | 0.51 | |||
30 | FSR 1345 | 248.34 | 10.02 | 2.3 | 8.9 | 0.51 | |||
31 | ESO 430-14 | 248.68 | −0.15 | 2.9 | 16.2 | 0.23 | |||
32 | FSR 1347 | 248.94 | −4.14 | 2.2 | 104.7 | 0.64 | |||
33 | Haffner 26 | 249.60 | 2.35 | 2.6 | 44.8 | 100.0 | 0.46 | ||
34 | Ruprecht 55 | 250.72 | 0.81 | 3.6 | 77.6 | 9.3 | 0.04 | y | |
35 | Ruprecht 59 | 253.07 | 0.93 | 4.0 | −5.0 | 6.3 | 0.00 | y | |
36 | ASCC 45 | 253.60 | −0.34 | 3.0 | 25.4 | 17.8 | 0.37 | ||
37 | Pup OB3 | 253.93 | −0.25 | 4.5 | 29.7 | 2.5 | 0.00 | y | 2 |
38 | Pismis 1 | 255.11 | −0.71 | 5.9 | 63.1 | 0.51 | |||
39 | Ruprecht 154 | 259.58 | −7.31 | 3.2 | 14.1 | 0.58 | |||
40 | FSR 1397 | 259.90 | 0.34 | 2.1 | 60.3 | 1.12 | |||
41 | DBSB 19 | 259.92 | −0.05 | 4.3 | 1.0 | 0.42 |
Notes. Columns 1 and 2: number and name of the star cluster. Columns 3–7 (l, b, dhc, vlsr and “age”): galactic longitudes, latitudes, heliocentric distances, radial velocities and ages of clusters. All values are taken from Kharchenko et al. (2013). Column 8 (dc–w): distance of the cluster to the wall of the supershell. y in the “Y/N” Col. 9 indicates if the formation of the cluster is very probably connected to the supershell. The last Col. 10 contains remarks; 1: the cluster lies inside the supershell. 2: the heliocentric distance of this cluster was changed from the catalogue value.
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