CORDIS Project
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This project investigates the infrared emission characteristics of large Polycyclic Aromatic Hydrocarbon molecules in the interstellar medium. By combining observational data with laboratory measurements and theoretical modeling, it aims to understand the origins and roles of these molecules in the universe.
Strong emission features dominate the IR spectra of the interstellar medium of the Milky Way, galaxies in the local Universe and out to redshifts of ~3.
These features are generally attributed to IR fluorescence of large Polycyclic Aromatic Hydrocarbon (PAH) molecules pumped by UV photons.
These species must be abundant, ubiquitous, and an important component of the ISM.
However, despite extensive experimental and theoretical efforts, no specific PAH or even classes of PAHs have been unambiguous…
UNIVERSITEIT LEIDEN
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