CORDIS Project
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This project investigates star formation in gas-rich galaxy centers, focusing on the Central Molecular Zone of nearby galaxies. By utilizing advanced observational techniques, it aims to understand the dynamics and processes influencing star formation in extreme environments characterized by high gas densities and inte…
Gas-rich galaxy centers like our own Milky Way's Central Molecular Zone (CMZ) are amongst the most extreme, yet poorly understood, environments for star formation.
These regions are affected by large-scale in- and out-flows of gas, by nuclear starburst and/or active galactic nuclei, which makes them unique laboratories in the local universe to study star formation at the highest gas and stellar mass densities, intense radiation fields, and short (<50 Myr) dynamical timescales. CMZs are compact (…
MAX-PLANCK-GESELLSCHAFT ZUR FORDERUNG DER WISSENSCHAFTEN EV
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