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Table 2

Modelled and observed binary parameters.

Primary Secondary

Teff (K) 140 000 ± 30 000 4500 ± 500
Radius (R) 0.13 ± 0.02 0.68 ± 0.03
Log g 4.5a
Inclination 90° ± 0.5°
0.91
Period (d) 0.6093 ± 0.0003
Peak-to-peak I-mag amplitude of irradiation effect 1.12 ± 0.07
Min. I-mag of sinusoidal region of lightcurve 16.80 ± 0.05b
Eclipse I-mag 18.40 ± 0.05c
Extinction-corrected min. V-mag of sinusoidal region 13.82 ± 0.08d
Extinction-corrected eclipse V-mag 17.36 ± 0.08e

Notes.

(a)

A fixed parameter in the modelling.

(b)

Measured value, not accounting for nebular contamination of roughly 10% at this phase.

(c)

Measured value, not accounting for nebular contamination of roughly 25% at this phase.

(d)

Corrected using the measured c(Hβ) = 2.42 ± 0.04, and a representative (V − I)0 = −0.4 for the nebular progenitor (Ciardullo et al. 1999).

(e)

Corrected using the measured c(Hβ) = 2.42 ± 0.04, and assuming that the modelled temperature is representative of the spectral type of the secondary (see text for details).

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