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.

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

New Radio Observations of Circinus X-1: A Summary

International Astronomical Union Colloquium Cambridge University Press (CUP) 164 (1998) 343-344

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