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Table 3.

Spectroscopically classified OB stars in W51.

# ID Field RA Dec J H K Sp Type (b)
(h m s) (° ′ ″) (mag) (mag) (mag)
1 OBS7slit08 IV 19 22 14.39 +14 03 09.0 11.58 ± 0.01 10.63 ± 0.01 10.04 ± 0.01 O3V–O5V
2 OBS6slit07 III 19 23 01.68 +14 16 40.4 13.68 ± 0.06 11.60 ± 0.04 10.34 ± 0.04 O3V–O5V
3 (a) OBS2slit17 II 19 23 42.85 +14 30 27.7 17.79 ± 0.03 13.58 ± 0.02 11.10 ± 0.02 O3V–O8V
4 OBS9slit17 III 19 23 07.76 +14 15 48.6 13.96 ± 0.02 12.34 ± 0.01 11.29 ± 0.01 O9V–B2V
5 OBS9slit08 III 19 23 02.65 +14 16 32.9 14.95 ± 0.02 12.67 ± 0.01 11.31 ± 0.01 O5V–O7V
6 OBS3slit16 II 19 23 41.03 +14 29 26.9 17.99 ± 0.05 14.34 ± 0.01 12.18 ± 0.01 O9V–B2V
7 OBS3slit17 II 19 23 44.79 +14 29 11.0 17.89 ± 0.04 14.99 ± 0.02 13.24 ± 0.02 B1V–B3V
8 OBS7slit24 IV 19 22 14.74 +14 04 43.3 14.50 ± 0.01 13.84 ± 0.01 13.46 ± 0.01 B8V–A3V
9 OBS8slit24 IV 19 22 18.02 +14 05 10.3 15.13 ± 0.01 14.08 ± 0.02 13.46 ± 0.02 B3V–B9V
10 OBS9slit23 III 19 22 59.25 +14 17 22.9 14.57 ± 0.01 14.12 ± 0.02 13.74 ± 0.02 B8V–A3V
11 OBS8slit23 IV 19 22 17.45 +14 04 56.3 14.55 ± 0.01 14.02 ± 0.01 13.76 ± 0.02 B3V–B7V
12 (c) OBS3slit15 II 19 23 42.99 +14 30 17.3 18.79 ± 0.08 16.65 ± 0.02 13.78 ± 0.01 B1V–B7V
13 OBS3slit09 II 19 23 37.36 +14 31 17.0 16.73 ± 0.02 15.05 ± 0.02 13.85 ± 0.03 B3V–B7V
14 OBS9slit15 III 19 23 04.51 +14 15 33.5 18.22 ± 0.05 15.45 ± 0.01 13.89 ± 0.01 B3V–B7V
15 OBS6slit16 III 19 23 07.49 +14 16 05.9 16.97 ± 0.02 15.47 ± 0.02 14.52 ± 0.02 B8V–A3V

16 OBS1slit17 II 19 23 38.50 +14 32 02.4 16.92 ± 0.02 13.84 ± 0.01 11.73 ± 0.01 YSO

LS1 (d) I 19 23 47.65 +14 36 39.1 8.10 ± 0.02 7.02 ± 0.06 6.24 ± 0.02 P Cygni SG
50 (e) II 19 23 42.88 +14 30 12.8 17.49 ± 0.03 14.09 ± 0.01 12.09 ± 0.01 O6.5V
57 (e) II 19 23 33.74 +14 29 53.8 16.66 ± 0.03 12.85 ± 0.01 10.64 ± 0.01 O4 V
61 (e) II 19 23 47.21 +14 29 43.6 15.16 ± 0.02 12.51 ± 0.02 O7.5V
W51d (e) II 19 23 39.92 +14 31 08.5 15.11 ± 0.02 12.32 ± 0.02 10.50 ± 0.03 O3V–O4V
IRS2E (e),(f) II 19 23 40.12 +14 31 05.9 16.70 ± 0.01 10.80 ± 0.01 YSO

Notes.

(a)

Source #44 in Figuerêdo et al. (2008).

(b)

Spectral types obtained by comparison with reference stars from Hanson et al. (1996, 2005) and Bik et al. (2005).

(c)

Not detected in the J-band in our catalogue, hence we used the value from the UKIDDS Galactic Plane Survey DR6 (Lucas et al. 2008).

(d)

Identified by Okumura et al. (2000) and spectrally modelled by Clark et al. (2009). Photometry taken from 2MASS.

(e)

Sources spectrally classified by Figuerêdo et al. (2008) and Barbosa et al. (2008). Photometry taken from our own data.

(f)

Photometry taken from Figuerêdo et al. (2008).

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