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.
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.