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.

X-Ray States and Radio Emission in the Black Hole Candidate XTE J1550–564

The Astrophysical Journal American Astronomical Society 554:1 (2001) 43-48

Authors:

S Corbel, P Kaaret, RK Jain, CD Bailyn, RP Fender, JA Tomsick, E Kalemci, V McIntyre, D Campbell-Wilson, JM Miller, ML McCollough

A jet model for the broadband spectrum of XTE J1118+480

Astronomy & Astrophysics EDP Sciences 372:2 (2001) l25-l28

Authors:

S Markoff, H Falcke, R Fender

The 1997 hard-state outburst of the X-ray transient GS 1354–64/BW Cir

Monthly Notices of the Royal Astronomical Society 91̽�� University Press (OUP) 323:2 (2001) 517-528

Authors:

C Brocksopp, PG Jonker, RP Fender, PJ Groot, M van der Klis, SJ Tingay

Radio flares and plasmon size in Cygnus X-3

(2001)

Authors:

RN Ogley, SJ Bell Burnell, RE Spencer, SJ Newell, AM Stirling, RP Fender

Microquasars: Hard X-ray/γ-ray emission

AIP Conference Proceedings AIP Publishing 558:1 (2001) 221-233

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