Fig. 7

Top: synthetic SEDs of the dust-free Cloudy models in the UV-optical regime. The input spectrum is the sum of the spectra of the gainer star, donor star, and hot spot with a temperature of 35 000 K (the last diluted according to the prescriptions of Appendix B). The fluxes are computed for a system distance of 300 pc. Bottom: same as top panel but for the different models A, B, and C (at different evolutionary times). The input spectra are in black from bottom to top (A, B, C).
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