Fig. 13
MOND fit of the rotation curve derived in the present paper, using the distance as a free parameter within the uncertainties of the Cepheids method (13.8 ± 1.5 Mpc). The dashed line is the Newtonian contribution of the gaseous disks (thin disk and extraplanar gas), the dotted line is the Newtonian contribution of the stellar disk (from de Blok et al. 2008), and the solid line is the best MOND fit.
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.