NOEMA CO(1-0) data for NGC 7479. Top left: moment-zero map. Top right: spectrum in a r = 3″ aperture centered on the continuum nucleus. The spectrum is fitted with three Gaussians for the host line profile. There is no outflow detection. Bottom left: center positions and their errors, from UV fitting a Gaussian model to individual velocity channels. The dotted line indicates the N–S direction of NGC 7479’s bar. Bottom right: position-velocity diagram. The pronounced bipolar structure in the PV diagram is ascribed to flow in the galaxy’s bar, and we adopt an upper limit for molecular outflow.