2003/02/17 by G. Matt, M. Guainazzi, R. Maiolino · 8 citations
Physics and Astronomy · #Absorption (acoustics) #Active galactic nucleus #Advanced X-ray Imaging Techniques #Astronomy #Astrophysical Phenomena and Observations #Astrophysics #Compton scattering #Galaxies: Formation, Evolution, Phenomena #Galaxy #Optics #Photon #Physics #Radiation #Reflection (computer programming) #Spectral line #astro-ph
paper · pdf · doi:10.1046/j.1365-8711.2003.06539.x
published as Mon.Not.Roy.Astron.Soc. 342 (2003) 422 · accepted for publication in MNRAS
arxiv created 2003/02/17 · openalex publication_date 2003/06/12 · arxiv updated 2009/12/01 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05
We discuss the properties of a small sample of type 2 Seyfert galaxies whose X-ray spectra changed appearance on time-scales of years, becoming reflection-dominated from Compton-thin, or vice versa. A reflection-dominated spectrum is usually taken as evidence of Compton-thick absorption, but we instead argue that such a spectrum is due to a temporary switching-off of the nuclear radiation. The observations discussed here may help to explain mismatches between optical and X-ray classifications, and provide new strong and direct evidence for the presence of more than one cold circumnuclear region in type 2 Seyfert galaxies.