Fig. 7
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Comparison with a sample of disks with masses >2 M⊙ in Orion (Kim et al. 2016). The top panels show the external FUV flux as a function of each spectral index, the XUE sources are shown with the colored dots and Kim et al. (2016) data with the gray crosses. The bottom panels show the empirical cumulative distribution functions for each index, the p values listed are the result of a Kolmogorov-Smirnov test.
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