Physics of ULIRGs with MUSE and ALMA: The PUMA project - III. Incidence and properties of ionised gas disks in ULIRGs, associated velocity dispersion, and its dependence on starburstiness

Free Access

Fig. C.2.

I07251 velocity maps and the 3D-Barolo disk kinematic best fit. In this target, the kinematic centre is shown with a black cross and the two ULIRG nuclei with red crosses. See Fig. C.1 for further details.

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.