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Large Polycyclic Aromatic Hydrocarbon (PAH) molecules are deeply interwoven in the fabric of the Universe and lock up ~15% of the elemental carbon in the interstellar medium (ISM) of galaxies. They dominate the mid-infrared emission characteristics of galaxies that can be used to trace star formation locally as well as in the early universe, they influence the phase structure of the ISM and the st ...
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