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.

Cygnus X-3 with ISO: investigating the wind

Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) 322:1 (2001) 177-186

Authors:

RN Ogley, SJ Bell Burnell, RP Fender

Powerful jets from black hole X-ray binaries in low/hard X-ray states

Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) 322:1 (2001) 31-42

X-ray states and radio emission in the black hole candidate XTE J1550-564

(2001)

Authors:

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

Correlated X-Ray Spectral and Timing Behavior of the Black Hole Candidate XTE J1550–564: A New Interpretation of Black Hole States

The Astrophysical Journal Supplement Series American Astronomical Society 132:2 (2001) 377-402

Authors:

Jeroen Homan, Rudy Wijnands, Michiel van der Klis, Tomaso Belloni, Jan van Paradijs, Marc Klein-Wolt, Rob Fender, Mariano Méndez

Spectral evidence for a powerful compact jet from XTE J1118+480

(2001)

Authors:

RP Fender, RM Hjellming, RPJ Tilanus, GG Pooley, JR Deane, RN Ogley, RE Spencer

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