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Table C.1.

Overview of the six young O stars observed in M17.

Interferometry
Mass Modelisation
Object CEN ID Component Optical mK Separation Phys. Separation Flux ratio χ2 Mass log(T) log(Lum) χ2
Spec. type (mas) (au) (M)
NGC6618-B189SW CEN 1a 1 O4Va 6.9b 17.6
2 7.79 ± 0.23 71.95 ± 2.49 120.88 ± 4.18 0.44 ± 0.04 14.2 - - - -
3 9.51 ± 0.55 4.40 ± 0.82 7.40 ± 1.37 0.09 ± 0.02 14.2 17.7
NGC6618-B189NE CEN 1b 1 O4Va 6.9b 25.3
2 7.21 ± 0.03 1.26 ± 0.02 2.12 ± 0.03 0.75 ± 0.01 2.7 26
NGC6618-B111 CEN 2 1 O4.5Vc 7.5 124.6
2 11.30 ± 0.83 17.26 ± 0.97 29.00 ± 1.64 0.03 ± 0.01 1.3 91
NGC6618-B98 CEN 3 1 O9Va 7.7 134.8
2 8.97 ± 0.24 1.01 ± 0.03 1.70 ± 0.06 0.31 ± 0.03 1.7 135
NGC6618-B0 OI 345 1 O6Va 7.4 71.8
2 10.89 ± 0.63 20.77 ± 1.51 34.88 ± 2.54 0.04 ± 0.01 1.6 72.0
3 12.40 ± 1.25 6.58 ± 2.09 11.05 ± 3.51 0.010 ± 0.005 1.6 75.3
NGC6618-B260 CEN 18 1 O6Va 7.8 84.3
2 10.69 ± 0.38 32.55 ± 2.45 56.69 ± 4.12 0.07 ± 0.01 2.3 84.1
3 12.05 ± 0.63 20.70 ± 4.76 34.76 ± 7.99 0.020 ± 0.005 2.3 85.6

Notes.

b

Combined magnitude of CEN 1a and 1b;

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