Evolution of X-ray spectra of Cygnus X-3 with radio flares

Details Evolution of X-ray spectra of Cygnus X-3 with radio flares Evolution of X-ray spectra of Cygnus X-3 with radio flares

2004-12-16

arxiv.org/abs/astro-ph/0412411v2

X-ray Timing 2003: Rossi and Beyond. AIP Conference Proceedings, Vol. 714, held 3-5 November, 2003 in Cambridge, MA. Edited by

Astronomy and Astrophysics

Astrophysics

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Scientific paper

10.1063/1.1781012

Cygnus X-3, among the X-ray binaries, is one of the brightest in the radio band, repeatedly exhibiting huge radio flares. The X-ray spectra shows two definite states, low (correspondingly hard) and high (correspondingly soft). During the hard state the X-ray spectra shows a pivoting behaviour correlated to the radio emission. In the high state the X-ray spectra shows a gamut of behaviour which controls the radio flaring activity of the source. The complete evolution of the X-ray spectra along with the radio flaring activity is reported here, for the first time for this source.

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