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Fig. 4.

image

Top: time of the merger as a function of the cutoff radius of the halo Rh, given in units of the scale radius of the disk Rd and assumed equal for the two galaxies. The initial tangential velocity here is fixed at 50 km s−1. Bottom: correlation between the time of the merger and the initial tangential velocity in the case of no IGM. The cutoff radii of the halos here are fixed at 70 Rd.

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