Free Access

Fig. 11

image

Mass budget within R ≃ 3 h in different types of dwarf galaxies: Irrs (blue diamonds, from Swaters et al. 2009), BCDs (black squares, from Lelli et al. 2014b), and TDGs (red points). For Irrs Mbar is estimated assuming both a “heavy disc” with (open symbols) and a “light disc” with (filled symbols). For BCDs the stellar mass is estimated from colour-magnitude diagrams of resolved stellar populations (see Lelli et al. 2014b).

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.