Astronomy and Astrophysics – Astronomy
Scientific paper
May 1995
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995ssrv...72..593m&link_type=abstract
Space Science Reviews, Volume 72, Issue 3-4, pp. 593-627
Astronomy and Astrophysics
Astronomy
11
Gamma Ray Astronomy, Gamma Rays, Production, Propagation, Pair Production, Light Curve, Spectral Emission, Stellar Radiation, Black Holes, Neutron Stars, Magnetic Fields, Accretion Disk Corona, Accretion Disk, Interstellar Medium, Eclipsing Binary Stars, X Ray Binaries: Sco X-1, Cyg X-3, Smc X-1, Her X-1, 4U0115+63, Cen X-3, Lmc X-4, Vela X-1, 4U1538-52, Gx 301-2, Stellar Orbits, Variability
Scientific paper
It is commonly accepted that candidates for very high energy γ-ray sources are neutron stars, binary systems, black holes etc. Close binary systems containing a normal hot star and a neutron star (or a black hole) form an important class of very high energy γ-ray sources. Such systems are variable in any region of the electromagnetic spectrum and they enable us to study various stages of stellar evolution, accretion processes, mechanisms of particle acceleration, etc. Phenomena connected with this class of very high energy γ-ray sources are discussed. Particular emphasis has been placed on the TeV energy region.
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