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.

The 1996 Outburst of GRO J1655-40: The Challenge of Interpreting the Multi-wavelength Spectra

(1998)

Authors:

RI Hynes, CA Haswell, CR Shrader, W Chen, K Horne, ET Harlaftis, K O'Brien, C Hellier, RP Fender

A radio survey of supersoft, persistent and transient X-ray sources in the Magellanic Clouds

(1998)

Authors:

RP Fender, K Southwell, AK Tzioumis

An Image of a Highly Relativistic Jet from a Large Flare in the X-Ray Binary Cyg X-3

International Astronomical Union Colloquium Cambridge University Press (CUP) 164 (1998) 351-352

Authors:

AJ Mioduszewski, RM Hjellming, MP Rupen, EB Waltman, GG Pooley, FD Ghigo, RP Fender

GRS 1915+105: Flares, QPOs and Other Events at 15 GHz

International Astronomical Union Colloquium Cambridge University Press (CUP) 164 (1998) 333-334

Authors:

GG Pooley, RP Fender

ISOCAM Observations of CYG X-3: Search for a Hot Stellar Wind

Chapter in Astrophysics and Space Science, Springer Nature (1998) 205-210

Authors:

RN Ogley, SJ Bell Burnell, RP Fender

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