Fig. 1
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Variations in the effective emission height of different tracers for a 3D disk demonstrated for HD 97048: (1) scattered-light as observed with SPHERE (Ginski et al. 2016), (2) PAH emission as observed with VISIR (Lagage et al. 2006), and (3) 13/12CO as observed with ALMA (Walsh et al. 2016). The inset on the bottom right is Fig. 4 from Lagage et al. (2006), demonstrating the 2D spatial distribution of the 8.6 μm PAH emission intensity of HD 97048.
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