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Fig. 1.

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Total mass of galactic components (dark matter, stars, gas) shown from top to bottom, with their half-mass radii, R0.5 (different colors represent different components, as per the legend); star formation rate (SFR); relative distance from the center of the group or cluster (blue, left y-axis), and the galaxy’s relative velocity (orange, right y-axis). The dashed vertical line represents the moment when the group merges with a nearby cluster.

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