The MURALES survey - IV. Searching for nuclear outflows in 3C radio galaxies at z < 0.3 with MUSE observations

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Fig. 4.

Comparison of the velocity measured at the 20th percentile of the whole [O III] line, v₂₀, and of the median velocity (v_50, wing) of the high-velocity wing on the nucleus. The dash-dotted line corresponds to a constant ratio of 1.6. This means that in our sample, v₂₀ would overestimate the outflow velocity.

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