Professor Rob Fender: Publications

An artist's impression of a relativistic jet propagating away from a black hole at close to the speed of light. Such jets are formed by the inner regions of the accretion flow: matter flowing inwards towards the black hole, via processes which are not yet fully understood. The accretion flow emits primarily in X-rays, the relativistic jet in the radio band: by combing observations in each band we can try and understand how such jets form and how much energy they carry away from the black hole.

A Comparison of Radio Emission From Neutron Star and Black Hole X-Ray Binaries

Chapter in The Neutron Star—Black Hole Connection, Springer Nature (2001) 261-266

Black-Hole States and Radio-Jet Formation

Chapter in Black Holes in Binaries and Galactic Nuclei: Diagnostics, Demography and Formation, Springer Nature (2001) 193-199

Energetics of Jets from X-Ray Binaries

Chapter in Microquasars, Springer Nature (2001) 69-77

Galactic Clues About the High-Energy Processes in BL Lac (AGN) Jets

Chapter in Astrophysical Sources of High Energy Particles and Radiation, Springer Nature (2001) 135-141

Authors:

S Markoff, H Falcke, PL Biermann, RP Fender

Jets in XRB Low/Hard States: Models of XTE J1118+480 Suggest a Strong Signature from Radio through X-Ray

Chapter in Microquasars, Springer Nature (2001) 289-290

Authors:

S Markoff, H Falcke, R Fender

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