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Fig. 3

image

LBQS0109: from left to right: [Oiii]λ5007 velocity map by Carniani et al. (2015b), ALMA continuum map at 3 mm, and narrow [OIII] emission tracing SF in the host galaxy (Carniani et al. 2016). White contours trace the flux map of CO(32) emission at the levels 3, 4 and 5σ. The red cross indicates the centroid of the H-band continuum emission. The cyan contours in the middle panel shows the flux map of the blue [Oiii]λ5007 wings collapsing the SINFONI cube over the velocity range − 1750 <v< − 1950 km s-1.

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