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Fig. 2

image

Example of an expansion curve, which is the expansion velocity of a shell as a function of the galactocentric radius. This curve is drawn for the shell number 1 and the gravitational potential of a de Vaucouleurs sphere (Sérsic sphere with index 4). The baryonic mass of the sphere is 1011M, and it has the effective radius of 5 kpc. The curve asymptotically reaches the value given by Eq. (10) indicated by the dashed line.

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