出版社：SISSA, Scuola Internazionale Superiore di Studi Avanzati
摘要：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
