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Table 4.

Summary of Ephemerides.

Set Year TAnom PA U deg/PA T0(WR in front) PS ω(T0)
IUE LW 1983.675 45582.4: 3.71:: 0.15:: −42:: −32:: 45582.4:: 3.4:: 271°
IUE SW 1983.673 45581.7: 3.74: −0.15: 42: 32: 45581.8: 4.1: 259°
IUE 1988.936 47504.0 3.74: −0.057: 110: 12: 47503.9: 3.87: 100°
IUE 1992.061 48645.38 3.61: −0.045 126 10.3 48644.30 3.71: 207°
IUE 1995.059 49740.17 3.72 −0.040 157 8.5 49739.15 3.81 199°
IUE Ps fixed 1995.058 49740.12 3.69 −0.037 170 7.8 49739.16 3.766 195°
Morel 1995.057 49739.59 3.71 −0.034 187 7.2 49738.83 3.79 175°
XMM-Newton 2010.785 55484.15 3.72 −0.034 187 7.2 55482.16 3.80 100°
BRITE 2015.888 57348.14 3.625 −0.075 83.6 15.6 3.789

Notes. Columns 3–10 are obtained from the model fits to the observed light curves and radial velocities. TAnom and T0 are, respectively, the time of periastron and the time when the WR is in front of the companion, and are given in units of JD−2400000. PA and PS are the anomalistic and sidereal periods, respectively and are given in days. The rate of change of the argument of periastron, , is given in radians per day; U is the apsidal period, given in days; deg/PA is given in degrees per anomalistic period; and ω(T0) is the argument of periastron at time T0 in degrees measured from elongation. The uncertainties in the values are discussed in Sect. 4.4.

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