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.

First observations of GRS 1915+105 with e-VLBI

Sissa Medialab Srl (2007) 092

Authors:

Anthony Rushton, Ralph E Spencer, Matthew Strong, Robert M Campbell, Simon Casey, Rob Fender, Michael Garrett, James CA Miller-Jones, Guy G Pooley, C Reynolds, Arpad Szomoru, Valeriu M Tudose, Zsolt Paragi

Jet-Powered Optical Nebulae From X-ray Binaries

Sissa Medialab Srl (2007) 059

Authors:

David M Russell, Rob Fender, Elena Gallo, James CA Miller-Jones, Christian R Kaiser

Jet-dominated advective systems of all mass scales

Sissa Medialab Srl (2007) 056

Authors:

Elmar Körding, Rob Fender

Looking for lobes in all the right places: Signatures of the interaction of microquasars with the ISM

Sissa Medialab Srl (2007) 057

Authors:

Sebastian Heinz, MA Aloy, Rob Fender, David M Russell

Monitoring LMXBs with the Faulkes Telescope

Sissa Medialab Srl (2007) 082

Authors:

Fraser Lewis, David M Russell, Rob Fender, Paul Roche

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