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

Open Access

Fig. B.3.

Relation of the cleaned merger-sensitive parameters (vertical axis in each tile) and the rotational support (horizontal axis in each tile). Red points show galaxies with log M_JAM ≥ 11. Blue points show galaxies with log M_JAM < 11. Full points show galaxies in environmental densities log ρ₁₀ ≥ −2. Empty points show galaxies in environmental densities log ρ₁₀ < −2.

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