A jet model for black-hole X-ray sources

Details A jet model for black-hole X-ray sources A jet model for black-hole X-ray sources

2007-02-27

arxiv.org/abs/astro-ph/0702710v1

PoSMQW6:039,2006

Astronomy and Astrophysics

Astrophysics

I Microquasar Workshop: Microquasars and Beyond, September 18-22 2006

Scientific paper

A jet model for Galactic black-hole X-ray binaries will be presented that appears to explain several observational characteristics. In particular, it explains the energy spectrum from radio to hard X-rays, the time-lags as a function of Fourier frequency, the increase of the variability amplitude (QPO and high frequency) with increasing photon energy, and the narrowing of the autocorrelation function with increasing photon energy. On the other hand, there are additional observational constraints that no model has tried to explain yet. It is important that we all try to address these constraints if we are to make any progress in understanding black-hole X-ray sources

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