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.

Modeling the X-ray contribution of XRB jets

New Astronomy Reviews Elsevier 47:6-7 (2003) 491-493

Authors:

Sera Markoff, Michael Nowak, Stéphane Corbel, Rob Fender, Heino Falcke

Moving relativistic large-scale X-ray jets in the microquasar XTE J1550−564

New Astronomy Reviews Elsevier 47:6-7 (2003) 477-480

Authors:

S Corbel, RP Fender, AK Tzioumis, JA Tomsick, JA Orosz, JM Miller, R Wijnands, P Kaaret

The connection between radio-quiet active galactic nuclei and the high/soft state of X-ray binaries

Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) 345:2 (2003) l19-l24

Authors:

Thomas J Maccarone, Elena Gallo, Rob Fender

Chandra Detections of Two Quiescent Black Hole X-Ray Transients

(2003)

Authors:

John A Tomsick, Stephane Corbel, Rob Fender, Jon M Miller, Jerome A Orosz, Michael P Rupen, Tasso Tzioumis, Rudy Wijnands, Philip Kaaret

First INTEGRAL observations of GRS 1915+105

(2003)

Authors:

DC Hannikainen, O Vilhu, J Rodriguez, S Brandt, NJ Westergaard, N Lund, I Mocoeur, Ph Durouchoux, T Belloni, A Castro-Tirado, PA Charles, AJ Dean, RP Fender, M Feroci, P Hakala, RW Hunstead, CR Kaiser, A King, IF Mirabel, GG Pooley, J Poutanen, K Wu, AA Zdziarski

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