Fig. 5.

Synthetic images of β Lyr A system for five different models: slab power-law, slab steady, wedge power-law, wedge steady, and nebula. The scale of grays corresponds to the monochromatic intensity Iv (in erg s−1 cm−2 sr−1 Hz−1). The wavelength is always λ = 545 mn and the orbital phase 0.25; α goes along east–west direction, and δ along north–south direction. It is worth noting that each model converged independently, but the outcomes are remarkably similar in terms of geometry.
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