MusE GAs FLOw and Wind (MEGAFLOW) - XII. Rationale and design of a Mg II survey of the cool circum-galactic medium with MUSE and UVES: The MEGAFLOW Survey

Open Access

Fig. 10.

Velocity offset Δv versus impact parameter b. The squares show the MEGAFLOW sample for galaxies within the impact parameter of b < 100 or b < 250 kpc. The triangles represent the MAGG sample from Dutta et al. (2020). The dotted line represents the escape velocity v_esc for the median halo mass of isolated galaxies M_h = 10^11.7 M_⊙ (Cherrey et al. 2025).

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.