Fig. 8.
Download original image
CO(1-0) spectra form the IRAM 30 m telescope (red, continuous line) and from CARMA (grey shaded), together with the HI emission (blue dashed line) integrated over the entire disc of the Tadpole galaxy. The HI spectrum contains only the emission of UGC 10214 (i.e. the emission from VV 29c has been excluded as described in Sect. 2.5). The HI flux is multiplied by a factor of 15 for better visibility.
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.