Astronomy and Astrophysics – Astrophysics
Scientific paper
2003-08-22
Astron.Astrophys.411:L405-L410,2003
Astronomy and Astrophysics
Astrophysics
6 pages, 5 colour figures, accepted for Astronomy and Astrophysics Letters, a special INTEGRAL issue
Scientific paper
10.1051/0004-6361:20031257
We present the first INTEGRAL results on Cyg X-3 from the PV phase observations of the Cygnus region. The source was clearly detected by the JEM-X, ISGRI and SPI detectors. The INTEGRAL observations were supported by simultaneous pointed RXTE observations. Their lightcurves folded over the 4.8 hour binary period are compatible with the mean RXTE/ASM and CGRO/BATSE light curves. We fit our broad band X-ray/Gamma-ray spectra with a physical model, which represents the first such published model for Cyg X-3. The main physical processes in the source are thermal Comptonization and Compton reflection with parameters similar to those found for black-hole binaries at high Eddington rates.
Beckmann Volker
Courvoisier Thierry J. -L.
Ebisawa Ken
Goldoni Paolo
Hakala Pasi
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