TEV emission from close binaries

Details TEV emission from close binaries TEV emission from close binaries

Jun 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993stin...9426268m&link_type=abstract

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Astronomy and Astrophysics

Astronomy

Binary Stars, Gamma Ray Astronomy, Gamma Rays, Hot Stars, Neutron Stars, Black Holes (Astronomy), Gamma Ray Spectra, Radio Sources (Astronomy)

Scientific paper

It is commonly accepted that candidates to very high energy gamma-ray sources are neutron stars (NS's), binary systems, black holes, etc. Close binary systems containing a normal hot star and a NS (or a black hole) form an important class of very high energy gamma-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 gamma-ray sources are discussed, the particular emphasis has been placed on the TeV region.

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