CORDIS Project
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This project explores the behavior of active galactic nuclei, focusing on the dusty gas surrounding supermassive black holes. It aims to characterize the mass distribution and kinematics of this dust, proposing a new model to explain the observed dusty winds and their impact on black hole activity.
Active galactic nuclei (AGN) represent the active growing phases of supermassive black holes.
For the first time, we are able to resolve the dusty gas on parsec scales and directly test our standard picture of these objects.
While this “unification scheme” relates the parsec-scale IR emission with a geometrically-thick disk, I have recently found that the bulk of the dust emission comes from the polar region of the alleged disk where gas is blown out from the vicinity of the black hole.
Along wi…
UNIVERSITY OF SOUTHAMPTON
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