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Fig. 8

image

Same as Fig. 5, but showing the effect of varying the morphology of the central object. Data points show results for equal-mass mergers of galaxies with reduced orbital energy rcir,p = 4/3 and halo spin parameter λ = 0.02. Open squares are used for mergers of pairs of E3 galaxies, while open circles identify Sb + Sb mergers.

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