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.

Magnetic field estimation in Cyg X-3's jet

New Astronomy Reviews Elsevier 42:9-10 (1998) 637-640

Authors:

RN Ogley, SJ Bell Burnell, RP Fender, GG Pooley, EB Waltman, M van der Klis

RXTE observations of Cygnus X-3

New Astronomy Reviews Elsevier 42:9-10 (1998) 629-632

Authors:

ML McCollough, CR Robinson, SN Zhang, BA Harmon, WS Paciesas, SW Dieters, RM Hjellming, M Rupen, AJ Mioduszewski, EB Waltman, FD Ghigo, GG Pooley, RP Fender, W Cui, S Trushkin

X-Ray Spectral Behavior of the Relativistic Jet Source Cygnus X-3

(1998)

Authors:

ML McCollough, CR Robinson, SN Zhang, BA Harmon, WS Paciesas, S Dieters, S Phengchamnan, RM Hjellming, M Rupen, AJ Mioduszewski, EB Waltman, FD Ghigo, GG Pooley, RP Fender, W Cui, S Trushkin

Infrared synchrotron oscillations in GRS 1915+105

Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) 300:2 (1998) 573-576

Authors:

RP Fender, GG Pooley

An Asymmetric Arcsecond Radio Jet from Circinus X-1

The Astrophysical Journal American Astronomical Society 506:2 (1998) l121-l125

Authors:

Robert Fender, Ralph Spencer, Tasso Tzioumis, Kinwah Wu, Michiel van der Klis, Jan van Paradijs, Helen Johnston

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