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.

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

Sissa Medialab Srl (2007) 098

Authors:

Valeriu M Tudose, Paolo Soleri, Rob Fender, Peter G Jonker, M van der Klis, Tasso Tzioumis, Ralph E Spencer

The LOFAR Transients Key Project

Sissa Medialab Srl (2007) 104

Authors:

Rob Fender, Ralph AMJ Wijers, Ben Stappers, Robert Braun, Michael W Wise, Thijs Coenen, Heino Falcke, Jean-Mathias Griessmeier, Michiel Van Haarlem, Peter G Jonker, Casey Law, Sera Markoff, Joseph Masters, James CA Miller-Jones, Rachel Osten, Bart Scheers, Hanno Spreeuw, John D Swinbank, Corina Vogt, Rudy Wijnands, Philippe Zarka

Linking Jet Emission, X-ray States and Hard X-ray Tails in the Neutron Star X-ray Binary GX 17+2

(2007)

Authors:

S Migliari, JCA Miller-Jones, RP Fender, J Homan, T Di Salvo, RE Rothschild, MP Rupen, JA Tomsick, R Wijnands, M van der Klis

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

Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) 379:3 (2007) 1108-1116

Authors:

DM Russell, RP Fender, PG Jonker

Tracing the jet contribution to the mid-IR over the 2005 outburst of GRO J1655-40 via broadband spectral modeling

(2007)

Authors:

S Migliari, JA Tomsick, S Markoff, E Kalemci, CD Bailyn, M Buxton, S Corbel, RP Fender, P Kaaret

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