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.

Evidence of a decrease of kHz quasi-periodic oscillation peak separation towards low frequencies in 4U 1728–34 (GX 354–0)

Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) 345:3 (2003) l35-l39

Authors:

S Migliari, M van der Klis, RP Fender

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First INTEGRAL observations of GRS 1915+105*

Astronomy & Astrophysics EDP Sciences 411:1 (2003) l415-l419

Authors:

DC Hannikainen, O Vilhu, J Rodriguez, S Brandt, NJ Westergaard, N Lund, I Mocœur, 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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High energy emission from microquasars

(2003)

Authors:

Rob Fender, Tom Maccarone

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Circular Polarisation Observations of SS433

Astrophysics and Space Science Springer Nature 288:1-2 (2003) 97-103

Authors:

DG McCormick, RE Spencer, RP Fender

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Circularly polarised radio emission from GRS 1915+105 and other X-ray binaries

Astrophysics and Space Science Springer Nature 288:1-2 (2003) 79-95

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Professor Rob Fender

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Evidence of a decrease of kHz quasi-periodic oscillation peak separation towards low frequencies in 4U 1728–34 (GX 354–0)

Authors:

First INTEGRAL observations of GRS 1915+105*

Authors:

High energy emission from microquasars

Authors:

Circular Polarisation Observations of SS433

Authors:

Circularly polarised radio emission from GRS 1915+105 and other X-ray binaries

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Professor Rob Fender

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Evidence of a decrease of kHz quasi-periodic oscillation peak separation towards low frequencies in 4U 1728–34 (GX 354–0)

Authors:

First INTEGRAL observations of GRS 1915+105*

Authors:

High energy emission from microquasars

Authors:

Circular Polarisation Observations of SS433

Authors:

Circularly polarised radio emission from GRS 1915+105 and other X-ray binaries