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BROADBAND EMISSION SPECTRA FROM THE CYGNUS X-3 JET IN THE SOFT SPECTRAL STATE.
- Source :
-
Astrophysical Journal . 2/1/2015, Vol. 799 Issue 2, p1-1. 1p. - Publication Year :
- 2015
-
Abstract
- In order to understand the main observational characteristics of the Galactic X-ray binary Cygnus X-3, we propose a radiation model in which high-energy electrons accelerate in the dissipation zone of a jet and produce nonthermal broadband emissions. Broadband spectral energy distributions are computed to compare the AGILE and Fermi LAT data with the multi-band data during soft X-ray spectral states. By fitting observations at different locations of the jet, we find that the emission region is rather compact and should be located at a distance of about one orbital radius. Our results can explain the current multi-frequency observations and also predict the TeV band emission. The model could be tested by a polarization measurement at IR band, and/or by a correlation study between the GeV and TeV bands once very-high-energy observations are available. [ABSTRACT FROM AUTHOR]
- Subjects :
- *GALACTIC X-ray sources
*CYGNUS X-3
*GAMMA rays
*BINARY stars
*GALAXIES
Subjects
Details
- Language :
- English
- ISSN :
- 0004637X
- Volume :
- 799
- Issue :
- 2
- Database :
- Academic Search Index
- Journal :
- Astrophysical Journal
- Publication Type :
- Academic Journal
- Accession number :
- 100758862
- Full Text :
- https://doi.org/10.1088/0004-637X/799/2/216