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Fig. 2

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Channel maps of CO(3–2) emission in the center of NGC 1566. Each of the 42 panels is 20′′  in size. Channels are separated by 10.15 km s-1. They are plotted from Vhel = 1302 (top left) to 1718.15 km s-1 (bottom right). The synthesized beam is 0.64′′× 0.43′′ (PA = 123°). The phase center of the observations (marked by a 4′′ cross) is given in Table 1. The grey scale is linear, between 1 and 30 mJy/beam. The central channels are saturated to better show the extent of the emission.

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