Table 1:
Photometry of the stars analyzed in the present paper. The stars are identified by their number in the list of Figer et al. (2002). Observed magnitudes are also from this source. A distance of 7.62 kpc is assumed (Eisenhauer et al. 2005), as well as a uniform extinction AK=2.8 in the K band (Stolte et al. 2002).
| Star |
ST |
mK |
MK |
| B1 |
WN8-9h |
11.11 |
-6.10 |
| F1 |
WN8-9h |
10.45 |
-6.76 |
| F2 |
WN8-9h |
11.18 |
-6.03 |
| F3 |
WN8-9h |
10.46 |
-6.75 |
| F4 |
WN7-8h |
10.37 |
-6.84 |
| F5 |
WN8-9h |
10.86 |
-6.35 |
| F6 |
WN8-9h |
10.37 |
-6.84 |
| F7 |
WN8-9h |
10.48 |
-6.73 |
| F8 |
WN8-9h |
10.76 |
-6.45 |
| F9 |
WN 8-9h |
10.77 |
-6.44 |
| F10 |
O4-6If+ |
11.46 |
-5.75 |
| F12 |
WN7-8h |
10.99 |
-6.22 |
| F14 |
WN8-9h |
11.22 |
-5.99 |
| F15 |
O4-6If+ |
11.27 |
-5.94 |
| F16 |
WN8-9h |
11.40 |
-5.81 |
| F18 |
O4-6I |
11.63 |
-5.58 |
| F20 |
O4-6I |
12.16 |
-5.05 |
| F21 |
O4-6I |
11.77 |
-5.44 |
| F22 |
O4-6I |
12.02 |
-5.19 |
| F23 |
O4-6I |
12.19 |
-5.02 |
| F26 |
O4-6I |
12.34 |
-4.87 |
| F28 |
O4-6I |
12.17 |
-5.04 |
| F29 |
O4-6I |
12.26 |
-4.95 |
| F32 |
O4-6I |
12.42 |
-4.79 |
| F33 |
O4-6I |
12.42 |
-4.79 |
| F34 |
O4-6I |
12.49 |
-4.72 |
| F35 |
O4-6I |
12.37 |
-4.84 |
| F40 |
O4-6I |
12.67 |
-4.54 |
Source LaTeX |
All tables |
In the text