Left: deep observations of NGC 5907 in the visible light showing the thin disc with the gigantic loops (from M08). Middle: one simulation of the loops at T = 8.0 Gyr with the M3L34G6 model, in which we assume a dust extinction screen affecting the stellar light density by a factor of 2.5 on both sides of the edge-on disc (see discussion in Sect. 6.1). Right: same model as middle panel shows all components with accounting for an extinction by a factor 12. The real extinction should be between the middle and right panel.
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