Differences in the physical properties of satellite galaxies within relaxed and disturbed galaxy groups and clusters

Open Access

Fig. 5.

Differences in the physical properties (colour, sSFR and metallicity) of the satellite galaxies belonging to relaxed (blue) and disturbed (red) clusters in clusters at low-redshift bin (0.1≤z<0.5). We also separate the satellite galaxies inside R₂₀₀ (left panels) and outside R₂₀₀ (right panels).

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