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INTEGRAL-RXTE observations of Cygnus X-1

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INTEGRAL-RXTE observations of Cygnus X-1

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Pottschmidt, K.; Wilms, J.; Chernyakova, M.; Nowak, M.A.; Rodriguez, J.; Zdziarski, A.A.; Beckmann, V.; Kretschmar, P.; Gleissner, T.; Pooley, G.G.; Martinez Nuñez, Silvia; Courvoisier, T.J.L.; Schönfelder, V.; Staubert, R.
Este documento es un/a artículo publicado, creado en: 2003
We present first results from contemporaneous observations of Cygnus X-1 with INTEGRAL and RXTE,made during INTEGRAL’s performance verification phase in 2002 November and December. Consistent with earlier results, the 3−250 keV data are well described by Comptonization spectra from a Compton corona with a temperature of kT ∼ 50−90 keV and an optical depth of τ ∼ 1.0−1.3 plus reflection from a cold or mildly ionized slab with a covering factor of Ω/2π ∼ 0.2−0.3. A soft excess below 10 keV, interpreted as emission from the accretion disk, is seen to decrease during the 1.5 months spanned by our observations. Our results indicate a remarkable consistency among the independently calibrated detectors, with the remaining issues being mainly related to the flux calibration of INTEGRAL.

    POTTSCHMIDT, K. ; Wilms, J. ; Chernyakova, M. ; Nowak, M.A. ; Rodriguez, J. ; Zdziarski, A.A. ; Beckmann, V. ; Kretschmar, P. ; Gleissner, T. ; Pooley, G.G. ; Martinez Nuñez, Silvia ; Courvoisier, T.J.L. ; Schönfelder, V. ; Staubert, R., 2003, INTEGRAL-RXTE observations of Cygnus X-1, Astronomy and Astrophysics, vol. 411, no. 1, p. L383–L388
http://www.aanda.org/articles/aa/pdf/2003/43/aaINTEGRAL26.pdf
distribuido bajo licencia Creative Commons de Reconocimiento-NoComercial 3.0 No adaptada

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