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Fig. 9


Integrated dust density predictions (i.e. extinctions in mag.) for the Orion complex for the same two distance slices as shown in Fig. 2 of Schlafly et al. (2015). Most of the extinction is at distances more than 300 pc. Orion A, Orion B, and λ Orionis are indicated by dashed lines (Lombardi et al. 2011) and the solid contours show the E(BV) = 0.5 mag from the 2D dust map of Schlegel et al. (1998; SFD), where the hatched area indicates lower reddening.

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