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.

Evolution of the radio - X-ray coupling throughout an entire outburst of Aquila X-1

(2010)

Authors:

JCA Miller-Jones, GR Sivakoff, D Altamirano, V Tudose, S Migliari, V Dhawan, RP Fender, MA Garrett, S Heinz, EG Körding, HA Krimm, M Linares, D Maitra, S Markoff, Z Paragi, RA Remillard, MP Rupen, A Rushton, DM Russell, CL Sarazin, RE Spencer

Fast infrared variability from a relativistic jet in GX 339-4

\mnras 404 (2010) L21-L25-L21-L25

Authors:

P Casella, TJ Maccarone, K O Brien, RP Fender, DM Russell, M van der Klis, A Pe Er, D Maitra, D Altamirano, T Belloni, G Kanbach, M Klein-Wolt, E Mason, P Soleri, A Stefanescu, K Wiersema, R Wijnands

Investigating the disc-jet coupling in accreting compact objects using the black hole candidate Swift J1753.5-0127

(2010)

Authors:

P Soleri, RP Fender, V Tudose, D Maitra, M Bell, M Linares, D Altamirano, R Wijnands, T Belloni, P Casella, JCA Miller-Jones, T Muxlow, M Klein-Wolt, M Garrett, M van der Klis

No evidence for black hole spin powering of jets in X-ray binaries

(2010)

Authors:

Rob Fender, Elena Gallo, David Russell

Fast infrared variability from a relativistic jet in GX 339-4

(2010)

Authors:

P Casella, TJ Maccarone, K O'Brien, RP Fender, DM Russell, M van der Klis, A Pe'er, D Maitra, D Altamirano, T Belloni, G Kanbach, M Klein-Wolt, E Mason, P Soleri, A Stefanescu, K Wiersema, R Wijnands

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