NGC 3516's ionized gas outflow is best described by a bicone viewed along one edge, with disk spirals lit by the AGN and radiatively accelerated clouds.
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The Shape of AGN-Driven Winds in the Seyfert Galaxy NGC 3516
NGC 3516's ionized gas outflow is best described by a bicone viewed along one edge, with disk spirals lit by the AGN and radiatively accelerated clouds.