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.

51��ing the X-ray hysteresis in GX 339-4: the disc and iron line over one decade

(2008)

Authors:

RJH Dunn, RP Fender, EG Koerding, C Cabanac, T Belloni

Polarised infrared emission from X-ray binary jets

(2008)

Authors:

DM Russell, RP Fender

Multiwavelength observations of the black hole candidate Swift J1753.5-0127

(2008)

Authors:

Paolo Soleri, Diego Altamirano, Rob Fender, Piergiorgio Casella, Valeriu Tudose, Dipankar Maitra, Rudy Wijnands, Tomaso Belloni, James Miller-Jones, Marc Klein-Wolt, Michiel van der Klis

Simultaneous X-ray/radio observations of Cir X-1

(2008)

Authors:

Paolo Soleri, Valeriu Tudose, Rob Fender, Michiel van der Klis

Searching for the signatures of jet-ISM interactions in X-ray binaries

(2008)

Authors:

James Miller-Jones, Christian Kaiser, Tom Maccarone, Rob Fender, Anna Kapińska, Katherine Gunn, David Russell, Catherine Brocksopp, Jennifer Sokoloski, Ben Stappers, Tom Muxlow

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