Abstract

Galaxy-wide winds of ionized gas have shown that AGN can terminate star formation in the most powerful radio galaxies at z 2, but these are rare objects and 1000 times brighter in the radio than typical dusty high-z starbursts. We have observed 50 high-z radio galaxies with the VLT/SINFONI IFU to explore the systematics of AGN-driven winds from the most powerful radio sources to sources with moderate radio power. We report on the latest results of this ongoing study.

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