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. 13.

REW ( $W_{r}^{2796}$ $W_{\mathrm{r}}^{2796}$ ) vs. impact parameter (b) for primary absorption-galaxy pairs within 100 kpc. The solid squares (circles) represent the pairs with only 1 galaxy (mulitple galaxies) within 100 kpc. Cherrey et al. (2025) investigates the $W_{r}^{2796} - b$ $W_{\mathrm{r}}^{2796}-b$ relation of isolated galaxies and its dependence with the physical properties of the host. The triangles represent the MAGG sample (Dutta et al. 2020).

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