Dynamics of the NGC 4636 globular cluster system - II. Improved constraints from a large sample of globular cluster velocities

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Fig. 16

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Number density profile of the blue and red GCs. The data from D+05 (their Table A3) are shown as crosses and dots for the blue and red GCs, respectively. The curves are the fits (cf. Eq. (11), Table 8) to the data, and the radial range is indicated by the arrow and the vertical lines.

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