Recurrent microblazar activity in cygnus x-1?
Aug, 2002
4 pages
Published in:
- Astron.Astrophys. 393 (2002) L61-L64
e-Print:
- astro-ph/0208495 [astro-ph]
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Abstract: (arXiv)
Recurrent flaring events at X- and soft gamma-ray energies have been recently reported for the galactic black hole candidate Cygnus X-1. The observed fluxes during these transient outbursts are far higher than what is observed in ``normal'' episodes. Here we suggest that the origin of this radiation is non-thermal and produced by inverse Compton interactions between relativistic electrons in the jet and external photon fields, with a dominant contribution from the companion star field. The recurrent and relatively rapid variability could be explained by the precession of the jet, which results in a variable Doppler amplification.- X-RAY BINARIES
- GAMMA-RAY OBSERVATIONS
- GAMMA-RAY THEORY
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