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X-Ray Properties of Black-Hole Binaries
Annual Review of Astronomy and Astrophysics
We review the properties and behavior X-ray binaries that contain an accreting black hole. The larger majority of such systems are X-ray transients, and many of them were observed in daily pointings with RXTE throughout the course of their outbursts. The complex evolution of these sources is described in terms of common behavior patterns illustrated with comprehensive overview diagrams for six selected systems. Central to this comparison are three X-ray states of accretion, which are revieweddoi:10.1146/annurev.astro.44.051905.092532 fatcat:2ehr4uivrjagng2ufnkmxdtqhm