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TeV and PeV gamma-ray emission from accreting pulsars
KIRALY, P ; MESZAROS, P
Astrophys. J.; (United States), 1988-10, Vol.333 (2), p.719-728
[Periódico revisado por pares]
Chicago, IL: University of Chicago Press
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Título:
TeV and PeV gamma-ray emission from accreting pulsars
Autor:
KIRALY, P
;
MESZAROS, P
Assuntos:
640102 - Astrophysics & Cosmology- Stars & Quasi-Stellar, Radio & X-Ray Sources
;
Astronomy
;
ATMOSPHERES
;
BINARY STARS
;
CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS
;
COSMIC RADIO SOURCES
;
COSMIC RAY SOURCES
;
COSMIC X-RAY SOURCES
;
Earth, ocean, space
;
ELECTROMAGNETIC RADIATION
;
Exact sciences and technology
;
GAMMA RADIATION
;
Gamma-ray sources
;
gamma-ray bursts
;
IONIZING RADIATIONS
;
MATHEMATICAL MODELS
;
MOTION
;
PULSARS
;
PULSES
;
RADIATIONS
;
ROTATION
;
STAR ACCRETION
;
STAR EVOLUTION
;
STAR MODELS
;
STARS
;
STELLAR ATMOSPHERES
;
STELLAR MAGNETOSPHERES
;
Stellar systems. Galactic and extragalactic objects and systems. The universe
;
Unidentified sources and radiation outside the solar system
;
X RADIATION
É parte de:
Astrophys. J.; (United States), 1988-10, Vol.333 (2), p.719-728
Descrição:
A corotating jet model for the high-energy gamma-ray emission of accreting pulsars is discussed which explains the pulse, orbital, and longer time scale behavior reported in the TeV and PeV ranges for Her X-1, 4U 0115 + 63, Vela X-1, and LMC X-4. This model is compatible with the present observational and theoretical understanding of the X-ray properties of these objects, and is based on the fact that the accreting pulsars confirmed so far as high-energy sources appear to have a nearly corotating magnetosphere. 60 references.
Editor:
Chicago, IL: University of Chicago Press
Idioma:
Inglês
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