Project

BOWIE

Centers of galaxies are home to supermassive black holes, often surrounded by large amounts of swirling gas and dust.

Where does all this material end up? Does it disappear forever inside a black hole or is it expelled from the galaxy in a powerful wind?

BOWIE aims to uncover the fate of this space dust by confronting observations from state-of-the-art telescopes with advanced numerical simulations.

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Illustration of dusty winds around an active galactic nucleus

BOWIE

Revealing Dusty Winds
Around Supermassive Black Holes

Today we know that almost all galaxies harbor supermassive black holes in their centers. Some are dormant, some active; some exposed, some hidden by dust. Active galactic nuclei can outshine all the stars in a galaxy combined.

Recent evidence points towards powerful dusty winds in some of the nearest active galaxies. In BlOWing In thE Wind — BOWIE — we aim to establish whether these winds are common and determine their properties.

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