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Fig. 3
XLFs for pre-main-sequence stars located in the Taurus Cluster (0.5–1 M⊙, Güdel et al. 2007; Owen et al. 2011) and the Orion Nebula Cluster (0.5–0.9 M⊙, Preibisch & Feigelson 2005). The dotted lines are drawn at the median X-ray luminosity for each corresponding XLF.
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