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.

The variable radio counterpart and possible large-scale jet of the new Z-source XTE J1701-462

(2007)

Authors:

RP Fender, M Dahlem, J Homan, S Corbel, R Sault, TM Belloni

The variability plane of accreting compact objects

(2007)

Authors:

EG Koerding, S Migliari, R Fender, T Belloni, C Knigge, I McHardy

The high energy emission of GRO J1655-40 as revealed with INTEGRAL spectroscopy of the 2005 outburst

(2007)

Authors:

MD Caballero-Garcia, JM Miller, E Kuulkers, M Diaz Trigo, J Homan, WHG Lewin, P Kretschmar, A Domingo, JM Mas-Hesse, R Wijnands, AC Fabian, RP Fender, M van der Klis

Evidence for a jet contribution to the optical/infrared light of neutron star X-ray binaries

(2007)

Authors:

DM Russell, RP Fender, PG Jonker

A highly polarised radio jet during the 1998 outburst of the black hole transient XTE J1748-288

(2007)

Authors:

Catherine Brocksopp, James Miller-Jones, Rob Fender, Ben Stappers

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