MOND implications for spectral line profiles of shell galaxies: shell formation history and mass-velocity scaling relations

Free Access

Fig. 5

Open with DEXTER Download original image

Radius r_10,c in units of the effective radius r_e (the function y_10,c(θ,ν) in Eq. (17)). Similar to Fig. 4. Measuring the circular velocity above r_10,c ensures that we can verify observationally the baryonic Tully-Fisher relation without introducing systematic errors that are too large.

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.