CORDIS Project
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This project aims to directly image the Cosmic Web, the vast network of matter in the universe, using bright quasars to illuminate gas emissions. It seeks to answer fundamental questions about galaxy formation by analyzing gas properties in both small and large scales.
Our cosmological model predicts that most of the matter in the universe is distributed in a network of filaments - the Cosmic Web - in which galaxies form and evolve.
Because most of this material is too diffuse to form stars, its direct imaging has remained elusive for several decades leaving fundamental questions still open, including: what are the morphological and kinematical properties of the Cosmic Web on both small (kpc) and large (Mpc) scales?
How do galaxies get their gas from the Cosmi…
UNIVERSITA' DEGLI STUDI DI MILANO-BICOCCA
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