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Table 9

Parameters of the stars in the sample that have been derived from those in Table 8 and the corresponding 1σ uncertainties.

Star log L R Mspec ΓEdd vesc v/vesc Dmom log Q0 log Q1
(L) (R) (M) (km s−1) (g cm s−2) (s−1) (s−1)
64066 5.510.07+0.11$5.51_{-0.07}^{+0.11}$ 13.20.9+0.6$13.2_{-0.9}^{+0.6}$ 13.32.0+8.2$13.3_{-2.0}^{+8.2}$ 0.650.23+0.11$0.65_{-0.23}^{+0.11}$ 36775+240$367_{-75}^{+240}$ 5.41.2+3.5$5.4_{-1.2}^{+3.5}$ 26.8+1.5$26.8_{\downarrow}^{+1.5}$ 49.3 48.4
A13 5.650.01+0.02$5.65_{-0.01}^{+0.02}$ 11.20.2+0.2$11.2_{-0.2}^{+0.2}$ 25.61.7+10.0$25.6_{-1.7}^{+10.0}$ 0.460.12+0.04$0.46_{-0.12}^{+0.04}$ 68545+210$685_{-45}^{+210}$ 3.10.7+0.2$3.1_{-0.7}^{+0.2}$ 27.80.2+0.1$27.8_{-0.2}^{+0.1}$ 49.4 48.8
62024 5.390.07+0.04$5.39_{-0.07}^{+0.04}$ 11.10.3+0.5$11.1_{-0.3}^{+0.5}$ 30.917.0+11.0$30.9_{-17.0}^{+11.0}$ 0.210.05+0.22$0.21_{-0.05}^{+0.22}$ 917410+190$917_{-410}^{+190}$ 1.150.2+0.9$1.15_{-0.2}^{+0.9}$ 27.50.3+0.2$27.5_{-0.3}^{+0.2}$ 49.0 48.2
B2 5.290.04+0.06$5.29_{-0.04}^{+0.06}$ 10.60.4+0.3$10.6_{-0.4}^{+0.3}$ 21.55.9+8.4$21.5_{-5.9}^{+8.4}$ 0.250.06+0.09$0.25_{-0.06}^{+0.09}$ 764160+180$764_{-160}^{+180}$ 1.30.4+0.8$1.3_{-0.4}^{+0.8}$ 25.70.5+0.7$25.7_{-0.5}^{+0.7}$ 48.9 48.1
B11 5.500.02+0.01$5.50_{-0.02}^{+0.01}$ 17.10.2+0.3$17.1_{-0.2}^{+0.3}$ 37.14.9+3.7$37.1_{-4.9}^{+3.7}$ 0.230.02+0.03$0.23_{-0.02}^{+0.03}$ 79870+49$798_{-70}^{+49}$ 1.690.19+0.06$1.69_{-0.19}^{+0.06}$ 26.00.2+1.1$26.0_{-0.2}^{+1.1}$ 48.9 47.2
A15 5.170.04+0.03$5.17_{-0.04}^{+0.03}$ 9.20.4+0.4$9.2_{-0.4}^{+0.4}$ 20.24.9+1.6$20.2_{-4.9}^{+1.6}$ 0.190.00+0.05$0.19_{-0.00}^{+0.05}$ 823130+17$823_{-130}^{+17}$ 1.460.04+0.27$1.46_{-0.04}^{+0.27}$ 25.50.2+0.2$25.5_{-0.2}^{+0.2}$ 48.7 47.8
A11 5.820.05+0.05$5.82_{-0.05}^{+0.05}$ 24.71.2+1.1$24.7_{-1.2}^{+1.1}$ 64.216.0+100.0$64.2_{-16.0}^{+100.0}$ 0.280.16+0.09$0.28_{-0.16}^{+0.09}$ 848160+690$848_{-160}^{+690}$ 1.60.8+0.6$1.6_{-0.8}^{+0.6}$ 25.20.2+0.6$25.2_{-0.2}^{+0.6}$ 49.2 47.6
N20 5.630.01+0.05$5.63_{-0.01}^{+0.05}$ 23.30.7+0.4$23.3_{-0.7}^{+0.4}$ 62.82.8+49.0$62.8_{-2.8}^{+49.0}$ 0.180.08+0.02$0.18_{-0.08}^{+0.02}$ 91519+370$915_{-19}^{+370}$ 1.750.44+0.08$1.75_{-0.44}^{+0.08}$ 27.210.07+0.58$27.21_{-0.07}^{+0.58}$ 48.7 46.5
N34 5.640.09+0.07$5.64_{-0.09}^{+0.07}$ 19.50.8+1.1$19.5_{-0.8}^{+1.1}$ 31.714.0+30.0$31.7_{-14.0}^{+30.0}$ 0.370.17+0.17$0.37_{-0.17}^{+0.17}$ 626240+360$626_{-240}^{+360}$ 2.81.2+1.2$2.8_{-1.2}^{+1.2}$ 27.40.2+6.5$27.4_{-0.2}^{+6.5}$ 49.2 48.0
S3 5.180.04+0.05$5.18_{-0.04}^{+0.05}$ 11.90.5+0.4$11.9_{-0.5}^{+0.4}$ 77.812.0+25.0$77.8_{-12.0}^{+25.0}$ 0.050.01+0.01$0.05_{-0.01}^{+0.01}$ 1539110+240$1539_{-110}^{+240}$ 0.160.05+0.09$0.16_{-0.05}^{+0.09}$ 24.5+0.5$24.5_{\downarrow}^{+0.5}$ 48.3 46.6
LP26 4.940.11+0.09$4.94_{-0.11}^{+0.09}$ 9.10.9+0.9$9.1_{-0.9}^{+0.9}$ 49.817.0+23.0$49.8_{-17.0}^{+23.0}$ 0.050.01+0.02$0.05_{-0.01}^{+0.02}$ 1413230+300$1413_{-230}^{+300}$ 0.60.5+1.2$0.6_{-0.5}^{+1.2}$ 24.4+1.8$24.4_{-\downarrow}^{+1.8}$ 48.0 46.3

Notes. Down arrows indicate upper limits. The quantities log Qi are the ionizing photon production rate of H and He I, for i = 0 and 1, respectively, and were calculated by integrating the SED of the best-fitting FASTWIND model.

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