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Fig. 6


Variation in the far-UV, 1280 Å (•) and 1600 Å (+ ) fluxes of Z And and AG Dra along their orbits as measured on the IUE spectra during their quiescent phases. The arrow points the flux from the spectrum in Fig. 1. The lines around φ = 0 and 1 represent Rayleigh attenuated light curves for models in keys. Orbital elements of Fekel et al. (2000b) were used.

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