From the Circumnuclear Disk in the Galactic Center to thick, obscuring tori of AGNs - Modeling the molecular emission of a parsec-scale torus as found in NGC 1068

Open Access

Fig. 8.

CO spectra. Upper panel: CO(6−5) model spectra of the southern and northern lobes. Lower panel: CO spectra toward the southern (left) and northern (right) lobe of the CND (from Requena-Torres et al. 2012). All spectra are convolved to the same angular resolution of 22.5″. The flux density is given in units of K, in T_mb.

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.