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QPO-jet relation in X-ray binaries

Published online by Cambridge University Press:  21 October 2010

Tomaso M. Belloni
Tomaso M. Belloni*
Affiliation:
INAF–Osservatorio Astronomico di Brera, Via E. Bianchi 46, I-23807 Merate, Italy email: tomaso.belloni@brera.inaf.it
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Abstract

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In the past years, a clear picture of the evolution of outbursts of black-hole X-ray binaries has emerged. While the X-ray properties can be classified into our distinct states, based on spectral and timing properties, the observations in the radio band have shown strong links between accretion and ejection properties. Here I briefly outline the association between X-ray timing and jet properties.

Keywords

accretionaccretion disksX-rays: binariesstars: outflows
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 5 , Highlights H15: Highlights of Astronomy , November 2009 , pp. 243 - 244
Copyright
Copyright © International Astronomical Union 2010

References

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