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.

A transient large-scale relativistic radio jet from GX 339−4

Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) 347:3 (2004) l52-l56

Authors:

E Gallo, S Corbel, RP Fender, TJ Maccarone, AK Tzioumis

An ultra-relativistic outflow from a neutron star accreting gas from a companion

(2004)

Authors:

Rob Fender, Kinwah Wu, Helen Johnston, Tasso Tzioumis, Peter Jonker, Ralph Spencer, Michiel van der Klis

An ultra-relativistic outflow from a neutron star accreting gas from a companion

Nature Springer Nature 427:6971 (2004) 222-224

Authors:

Rob Fender, Kinwah Wu, Helen Johnston, Tasso Tzioumis, Peter Jonker, Ralph Spencer, Michiel van der Klis

High Energy Emission from Microquasars

Chapter in Cosmic Gamma-Ray Sources, Springer Nature 304 (2004) 205-223

Authors:

Rob Fender, Tom Maccarone

Towards a Unified Description of the Jet-Accretion Coupling in Stellar and Super Massive Black Holes

Progress of Theoretical and Experimental Physics Oxford University Press (OUP) 155 (2004) 83-86

Authors:

Elena Gallo, Rob Fender, Tom Maccarone, Peter Jonker

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