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Table 3

Final used distances and associated errors, reddening parameters and derived stellar radii.

Source d(kpc) ed (kpc) E(BV) RV R* (R)
HD 66811 0.46 0.1 0.04 3.1 18.6
0.73 0.14 0.04 3.1 29.7
Cyg OB2#11 1.72* 1.745 3.1 23.15
HD 210839 0.62* 0.485 3.1 13.35
HD 152408 1.68 0.4 0.5 2.98 30.0
HD 151804 1.8 0.4 0.38 3.13 36.0
HD 149404 1.3 0.3 0.68 3.4 37.0
HD 30614 0.789 0.1 0.25 3.5 20.70

HD 37128 0.342 0.1 0.413 3.1 24.68
HD 38771 0.4 0.1 0.04 3.1 23.0
HD 154090 1.096 0.25 0.59 2.7 39.0
HD 193237 1.7 0.2 0.58 3.1 97.14
HD 24398 0.303* 0.30 2.9 21.12
HD 169454 2.13* 1.13 3.19 98.2
HD 152236 1.64 0.4 0.7 3.18 104.0
HD 41117 1.5 0.2 0.415 3.05 61.0
HD 194279 1.71* 1.23 3.2 78.4
HD 198478 0.83 0.1 0.51 3.0 35.8
HD 80077 2.55* 1.5 3.2 167.0
HD 53138 1.135 0.25 0.01 3.2 65.0
CyOB2#12 1.75 0.16 3.38 3.0 240.0
0.85* 3.38 3.0 116.7

HD 24912 0.854 0.1 0.3 3.18 23.4
HD 36861 0.27* 0.073 5.0 7.8
HD 37043 0.5 0.1 0.035 5.0 17.9

HD 149757 0.165 0.023 0.29 2.88 8.9
HD 149438 0.167 0.023 0.012 2.8 5.65

Notes. Sources are sorted as in Table 1. Asterisked values in the distance column correspond to Gaia DR2 distances, and the two values for HD 66811 and Cyg OB2#12 refer to different alternatives for these sources (see Sect. 2.4), quoted with their associated asymmetric errors. Some parameters have been modified from the initial values found in theliterature (see Table 5) by the de-reddening procedure (see Sect. 3).

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