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Table B.1

Results of the toy model for an orbit with eccentricity e=0.36.

Case (1) Primary (2) Secondary (3) αper R (4) αap R (5) r1per R (6) r2per R (7) r1ap R (8) r2ap R (9) V1per km s−1 (10) V2per km s−1 (11) T1per keV (12) T2per keV (13) V1ap km s−1 (14) V2ap km s−1 (15) T1ap keV (16) T2ap keV (17)
*1 O7–9III O7–9III 50.69 107.71 25.34 25.34 53.86 53.86 1037 1037 3.15 3.15 1803 1803 9.52 9.52
*2 B0I O7–9III 49.67 105.56 23.99 25.69 50.97 54.59 1056 3.27 607 1813 1.08 9.62
3 B0I B0I 48.62 103.31 24.31 24.31 51.66 51.66 618 618 1.12 1.12
*4 O9I O7–9III 54.06 114.88 28.83 25.23 61.27 53.61 311 1031 0.28 3.11 1110 1800 3.61 9.49
*5 O9I B0I 53.17 112.99 29.27 23.91 62.19 50.81 332 0.32 1121 604 3.68 1.07
*6 O9I O9I 57.06 121.25 28.53 28.53 60.63 60.63 296 296 0.26 0.26 1102 1102 3.56 3.56
*7 WN7 O7–9III 55.65 118.26 40.28 15.37 85.60 32.66 1125 176 4.95 0.09 1259 1357 6.20 5.39
*8 WN7 B0I 54.82 116.48 40.42 14.40 85.88 30.60 1126 4.96 1259 96 6.20 0.03
*9 WN7 O9I 58.49 124.30 40.73 17.76 86.55 37.75 1128 4.97 1260 656 6.21 1.26
*10 WN7 WN7 59.86 127.21 29.93 29.93 63.60 63.60 1039 1039 4.22 4.22 1217 1217 5.80 5.80
*11 WN7 WN8 64.18 136.37 21.89 42.29 46.51 89.86 918 843 3.30 2.78 1158 988 5.25 3.82
*12 WN8 O7–9III 60.57 128.70 50.58 9.99 107.48 21.23 887 3.08 1009 767 3.98 1.72
13 WN8 B0I 59.86 127.21 50.54 9.32 107.40 19.81 887 3.08 1009 3.98
*14 WN8 O9I 62.99 133.86 51.39 11.60 109.21 24.65 891 3.11 1011 83 4.00 0.02
*15 WN8 WN8 67.98 144.45 33.99 33.99 72.22 72.22 778 778 2.37 2.37 956 956 3.58 3.58
*16 WNVL O7–9III 74.74 158.83 56.15 18.59 119.32 39.50 539 0.85 123 1552 0.06 7.05
17 WNVL B0I 74.28 157.85 56.74 17.54 120.57 37.27 127 316 0.06 0.29
18 WNVL O9I 76.36 162.27 55.40 20.96 117.73 44.55 118 834 0.05 2.04
19 WNVL WN7 77.18 164.00 41.32 35.85 87.81 76.19 1094 4.68 9 1244 6.05
20 WNVL WN8 79.87 169.72 29.84 50.03 63.41 106.30 885 3.06 1008 3.98
21 WNVL WNVL 88.99 189.11 44.50 44.50 94.56 94.56 35 35

Notes. The notation follows that of Table 3 with subscripts “ap” and “per” denoting values at apastron and periastron, respectively. Cases marked with an asterisk represent configurations that can reproduce the observed spectrum.

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