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Variable Source of High Energy Gamma-Ray Radiation Cygnus X-3

2010/05/06 by A. M. Galper, Galper, A. M., B. I. Luchkov +4
Physics and Astronomy · #Astrophysical Phenomena and Observations #Astrophysics of Galaxies (astro-ph.GA) #FOS: Physical sciences #Gamma-ray bursts and supernovae #High Energy Astrophysical Phenomena (astro-ph.HE) #Instrumentation and Methods for Astrophysics (astro-ph.IM) #Pulsars and Gravitational Waves Research #astro-ph.GA #astro-ph.HE #astro-ph.IM

paper · pdf · doi:10.48550/arxiv.1005.1012

2 pages, 1 figure

arxiv created 2010/05/06 · openalex publication_date 2010/05/06 · arxiv updated 2010/05/07 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28

Abstract

Long observation (1972 - 2009) of the powerful discrete source in Galaxy Cygnus X-3 discovered its main properties and let to develop a real model of this unique object. It is short binary system with 4.8 hour orbital period including relativistic object (neutron star or black hole) and massive star. Source most activity is seen in gamma-rays from tens MeV to thousands TeV.

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