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Fig. 11

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Scenario for V505 Ori. The vertical black line marks the rotation axis, while the inclined black line marks the viewing horizon on the stellar disk. The dashed blue line marks the magnetic axis. The red lines represent the accretion funnels hitting the star near to the magnetic axis and creating the hot accretion spot there. The (opaque) disk is shown in red here and the dotted black line marks the part of the star, which is blocked from view by the disk. The (asymmetric) pink areas mark less dense parts of the disk, which lead only to reddening of the passing light. Top: brightness maximum. Here, the accretion spot can be fully seen, leading to the highest veiling and some imprint of the accretion funnel in the spectrum. Bottom: brightness minimum. Here, only a small part of the accretion spot can be seen, and the accretion funnel cannot be viewed.

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