Fig. 1
Kinematics of NGC 1400 (left) and NGC 1407 (right) based on the sample of GCs from the SLUGGS database. From top to bottom: LOS velocity of the GCs in kms-1; velocity dispersion in kms-1 calculated in a given bin and the s3 and s4 parameters, which describe symmetric and asymmetric departures from the Gaussian, respectively. The vertical dotted line in both plots denotes one effective radius. See text for details.
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