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Fig. 10

image

Top: distribution of Virgo galaxies, as well as the initial galaxy models and remnants in the μeffreff plane. Bottom: distribution of Virgo galaxies, as well as the initial galaxy models and remnants in the Mr − ⟨μeff plane. The points for the initial and remnant galaxies are the mean values averaged over different projection angles (edge on = 90°, 67.5°, 45°, 22.5°, face on = ) along the x-axis and along the y-axis. The error bars span over the range from the minimum to the maximum value of the projections.

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