Very extended cold gas, star formation and outflows in the halo of a bright quasar at z > 6

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Fig. 6

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Distribution of dynamical time scales (τ_dyn = R/v, where R is the projected distance from the central quasar and v is the outflow velocity) within the outflow, obtained for the individual outflowing clumps as described in Sect. 3.4 and in Appendix C.

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