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Table 2

Spectroscopically observed stars.

ID RA (J2000) Dec (J2000) J H KS Spectral type AKS Distance
[h      m      s] [°      ′      ′′] [mag] [mag] [mag] [mag] [kpc]

Star cluster candidates:
1 18 50 17.398 +00 22 04.77 14.843 13.101 12.204 B1 V 1.83 3.69
3 18 50 19.420 +00 21 41.15 14.089 12.051 10.925 O9 V 2.21
4 18 50 16.434 +00 21 31.44 14.316 12.671 11.839 B0 V 1.74
5 18 50 16.555 +00 21 21.69 13.817 11.987 11.033 O9.5 V 1.95
6 18 50 16.500 +00 21 07.01 13.976 12.193 11.162 B0 V 1.96
7 18 50 17.481 +00 20 56.26 14.307 12.438 11.400 O9.5 V 2.03
8 18 50 15.903 +00 20 44.31 13.821 12.261 11.317 O9.5–B0 V 1.76
9 18 50 16.185 +00 20 35.77 14.958 12.848 11.603 O9.5 V 2.33
11 18 50 23.945 +00 19 57.52 13.762 11.880 10.995 O9 V 1.95
12 18 50 23.091 +00 19 47.64 13.535 11.496 10.456 O9 V 2.15
13 18 50 22.271 +00 19 28.18 15.505 13.357 12.205 B0 V 2.29
15 18 50 17.303 +00 20 59.01 14.889 12.955 11.843 B0 V 2.12
16 18 50 16.837 +00 21 12.35 13.697 12.006 10.999 B0 V 1.90
17 18 50 17.036 +00 21 46.69 14.326 12.485 11.471 B0 V 2.00
19 18 50 13.554 +00 21 03.23 13.606 11.895 10.981 B0 V 1.84
20 18 50 12.329 +00 20 46.68 14.829 13.25 11.96 B0 V 2.00
21 18 50 10.573 +00 20 25.64 13.727 12.028 11.071 O9.5 V 1.87
s01 18 50 17.623 +00 21 30.65 10.812 8.893 7.839 A2 I 1.89
s03 18 50 15.408 +00 20 58.07 9.232 6.625 5.299 M2 I 1.99
s04 18 50 15.620 +00 21 07.46 9.563 6.984 5.649 M2 I 1.98
s05 18 50 14.117 +00 22 39.56 9.300 6.477 4.938 M1 I 2.25

Fore-/background stars:
2 18 50 21.558 +00 21 52.31 13.720 12.636 12.054 A0 V 1.10 1.18
10 18 50 14.005 +00 20 06.94 11.281 9.966 9.472 G9–K2 III 0.74 1.32
14 18 50 20.709 +00 21 17.59 10.994 9.638 9.065 G9–K2 III 0.82 1.06
18 18 50 15.788 +00 21 46.06 10.752 9.775 9.391 G0 III 0.61 0.81
22 18 50 10.445 +00 21 03.80 10.499 9.603 9.143 G9–K2 III 0.44 1.31
23 18 50 08.513 +00 22 11.42 11.019 9.528 8.94 G6 III 1.01 0.67
s02 18 50 28.354 +00 21 13.44 11.348 8.935 7.818 K–M I–III ···    ···   

Notes. Equatorial coordinates, near-infrared magnitudes (J, H, and KS), and spectral classification are given for all stars. For those stars with determined luminosity class are given also the estimated extinction and distance.

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