DENSE MOLECULAR GAS AROUND PROTOSTARS AND IN GALACTIC NUCLEI: PDRS AND XDRS

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Abstract

The chemical and thermal structure of dense gas irradiated by FUV and X-ray photons is explored. The relevance of these so-called PDRs (FUV) and XDRs (X-ray) for AGN and YSOs is discussed. Observational line diagnostics and chemical tracers are summarized.

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