Diagnostics of irradiated dense gas in galaxy nuclei

2006/10/13 by R. Meijerink, M. Spaans, F. P. Israel · 16 citations
Physics and Astronomy · #Active galactic nucleus #Astronomy #Astrophysical Phenomena and Observations #Astrophysics #Astrophysics and Star Formation Studies #Galaxies: Formation, Evolution, Phenomena #Galaxy #Nuclear physics #Physics #Radiation #Stars #astro-ph

paper · pdf · doi:10.1051/0004-6361:20066130

34 pages, 47 figures, accepted by A&A, a version with all figures is available at http://www.strw.leidenuniv.nl/~meijerin/grid/GridCodes_printer.pdf

arxiv created 2006/10/13 · openalex publication_date 2006/10/16 · arxiv updated 2009/12/01 · openalex created_date 2022/08/25 · openalex updated_date 2026/07/31

Abstract

Aims.The nuclei of active galaxies harbor massive young stars, an accreting central black hole, or both. In order to determine the physical conditions that pertain to molecular gas close to the sources of radiation, numerical models are constructed.

Citations

• Diagnostics of irradiated gas in galaxy nuclei

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