Roland Svensson
Published 1996-05-15, updated 1996-05-17Version 2
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.
Comments: 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
Gamma-ray emission from Outer-Gap of pulsar magnetosphere
X-ray and gamma-ray observations of millisecond pulsars
Gamma-ray emission expected from Kepler's SNR
