Fig. 8
Comparison of integrated H i linewidth W50 to FWHM of the Hα integrated velocity dispersion 
. The dashed line indicates the one-to-one relation. For LARS 6, (encircled point) we plot as W50, a preliminary result based upon VLA C-configuration interferometry, as the beam of the GBT profile (used to derive W50 in Paper III) is too broad to separate LARS 6 from a neighbouring galaxy.
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.