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A model for (quasi )periodic multi wavelength photometric variability in young stellar objects

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Figure

Figure 1. Three-color plots of the star and inner disk region represented by Model 1 having two hot spots due to accretion that illuminate a truncated disk with an inner(warp (see Table 1 for details)
Table 1Model Parameters
Figure 2. Model light curves for the periodic category over two rotations; see Table 1 for a detailed description
Table 2Statistics for the Periodic Models
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