Dense Molecular Gas around Protostars and in Galactic Nuclei: PDRs and XDRs

Details Dense Molecular Gas around Protostars and in Galactic Nuclei: PDRs and XDRs Dense Molecular Gas around Protostars and in Galactic Nuclei: PDRs and XDRs

Jan 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005ap%26ss.295..239s&link_type=abstract

Astrophysics and Space Science, Volume 295, Issue 1-2, pp. 239-248

Astronomy and Astrophysics

Astrophysics

6

Galaxies: Ism, Galaxies: Agn, Infrared: Ism: Lines And Continuum, Ism: Atoms And Molecules

Scientific paper

The chemical and thermal balance 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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