1996/05/15 by Roland Svensson, Svensson, Roland
Physics and Astronomy · #Astrophysical Phenomena and Observations #Astrophysics (astro-ph) #Dark Matter and Cosmic Phenomena #FOS: Physical sciences #Particle Detector Development and Performance #astro-ph
paper · pdf · doi:10.48550/arxiv.astro-ph/9605078
6 pages; l-aa style; 6 postscript figures; Proceedings of 3rd Compton Gamma-Ray Observatory Symposium, Munich, 1995; Figure 5 is changed to the correct one
openalex publication_date 1996/05/15 · arxiv created 1996/05/17 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28
X-ray and gamma-ray observations of Seyfert 1 galaxies are briefly reviewed. Both thermal and non-thermal model for X-ray and gamma-ray emission are discussed. Particular attention is given to various disc-corona models including both homogeneous and inhomogeneous (patchy) corona models. Recent work on exact radiative transfer in such geometries are reviewed.