Size and Kinetic Luminosity of Low Redshift Quasar Outflows

Astronomy and Astrophysics – Astronomy

Scientific paper

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Scientific paper

Over the past several months the new UV spectrograph aboard HST is giving us high quality data of AGN outflows, aka warm absorbers to the X-ray community. I will describe very new results from our program that aim at finding the size, kinetic luminosity and chemical abundances of these outflows.
We acknowledge support from NASA through HST program (11686), and from NSF grant AST 0837880.

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