U-band study of the accretion properties in the σ Orionis star-forming region

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Fig. C.1

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SEDs of four EV disks and 2 TD. The squares shows the observed fluxes (see Table C.2). The lines plot the model atmosphere from Allard et al. (2000) at the appropriate T_eff, log g = 4.0, normalized to the J band. Each panel gives the name of the star (see Table C.1) and the mass accretion rate.

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