Discovery of molecular gas fueling galaxy growth in a protocluster at z = 1.7

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Fig. 4.

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FRII host galaxy (a0) line velocity map (moment 1, with respect to the line central frequency of the fit marked by the vertical dotted black line in Fig. 2). North is up, and east is to the left. The open black ellipse is the restoring beam. The VLA contours as in Fig. 1 are reported in black.

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