Origin of the differences in rotational support among early-type galaxies: The case of galaxies outside clusters

Open Access

Fig. B.2.

Investigated merger-sensitive parameters as functions of the rotational support (vertical axis in each tile) and the ρ₁₀ environmental density (horizontal axis in each tile). We point out again that our sample does not contain galaxies in clusters. See Fig. 1 for an explanation of the meaning of the colors of the points.

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