Repositorio Académico de la Universidad de Chile
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Excitation of CO molecules in diffuse gas over cosmic history
We studied the physical conditions in the local interstellar medium (ISM) and at high redshift by fitting observed column densities of CO and H-2 rotational levels and C i fine-structure levels using photodissociation models calculated with the Meudon PDR code. We analysed CO absorption systems in 2
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