Fig. 2
Deprojected F814W image of ESO 320-G030 assuming an inclination of 43° and a PA of 133°. In the left panel, the central region is saturated to make visible the primary bar and the external spiral arms (pseudoring). The right panel shows the secondary bar and spiral structure present in the central 5 kpc. The contours represent the deprojected CO(2−1) emission. The diagonal white line in the left panel corresponds to the gap between the two HST/ACS detectors.
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