Linking nearby stellar streams to more distant halo overdensities

Free Access

Fig. 5.

Same as Fig. 3, but now for EriPhe. We note that no line-of-sight velocities are available for its members, so the right panel depicts a prediction of what to expect if EriPhe has a progenitor in common with the nearby halo substructures described in Sect. 2.

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.