Fig. 10

Overlays of the spatially unresolved H i (Morganti et al. 2003b) spectrum and the 12CO(1-0) and 12CO(2-1) spectra (with the continuum subtracted) toward the AGN, eastern jet, and disk regions of 3C 293. The CO spectra correspond to the regions of the AGN (top panels), jet (2nd row), and 12CO(1-0) and 12CO(2-1) emission disks (3rd row). The green-shaded area marks the area of the H i absorption that cannot be attributed to rotation around the AGN. Fluxes are in arbitrary units. Velocities are given with respect to .
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