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Fig. 3.

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Schematic illustration of the wind model composed of a central point source (orange) and a bipolar outflow with the radius Ro (red). The central source emits Lyα photons, following a Gaussian profile with a width σSrc. The bipolar outflow is characterized by the H I column density NH I, the opening angle θo, Wind (increasing from the +z-axis, as the blue solid arrow), and the expansion velocity vexp parameters. The inner radius of the outflow Ri is fixed at 0.1 Ro. As the wind model is symmetric about the z-axis, the line of sight angle θLOS is the angle from the +z-axis following the orange arrow, and thus with θLOS = 0° meaning observing in the direction of the outflow, and θLOS = 90° representing the equatorial view.

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