Fig. 7.
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Radiative age versus offset from the galaxy disc for the plasma in the stripped tail. Solid line shows the best-fit linear relationship (trad = m × ℓ + b) and the shaded regions show 1× and 2× the best-fit scatter. We also list the projected plasma velocity determined from the slope of the relation. Radiative ages are estimated assuming a minimum-loss magnetic field strength.
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