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Relativistic Jet from Black Hole

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.

Professor Rob Fender

Professor of Astrophysics

Research theme

  • Astronomy and astrophysics

Sub department

  • Astrophysics

Research groups

  • Hintze Centre for Astrophysical Surveys
  • MeerKAT
  • Pulsars, transients and relativistic astrophysics
  • Rubin-LSST
  • The Square Kilometre Array (SKA)
  • Gamma-ray astronomy
Rob.Fender@physics.ox.ac.uk
Telephone: 01865 (2)73435
Denys Wilkinson Building, room 712
  • About
  • Publications

Infrared synchrotron oscillations in GRS 1915+105

(1998)

Authors:

RP Fender, GG Pooley

MERLIN observations of GRS 1915+105 : a progress report

(1998)

Authors:

RP Fender, ST Garrington, DJ McKay, TWB Muxlow, GG Pooley, RE Spencer, AM Stirling, EB Waltman

Infrared photometry and spectroscopy of the supersoft X-ray source RX J0019.8+2156 (= QR And)

(1998)

Authors:

H Quaintrell, RP Fender

Radio observations of IRAS selected southern hemisphere classical Be stars

(1998)

Authors:

JS Clark, IA Steele, RP Fender

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

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