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91探花
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

Orbital, precessional and flaring variability of Cygnus X-1

(1999)

Authors:

C Brocksopp, RP Fender, V Larianiov, VM Lyuty, AE Tarasov, GG Pooley, WS Paciesas, P Roche

Quenching of the radio jet during the X-ray high state of GX 339-4

(1999)

Authors:

Robert Fender, Stephane Corbel, Tasso Tzioumis, Vince McIntyre, Duncan Campbell-Wilson, Mike Nowak, Ravi Sood, Richard Hunstead, Alan Harmon, Philippe Durouchoux, William Heindl

MERLIN observations of relativistic ejections from GRS 1915+105

Monthly Notices of the Royal Astronomical Society 91探花 University Press (OUP) 304:4 (1999) 865-876

Authors:

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

High resolution optical and infrared spectroscopic observations of Cir X-1

(1999)

Authors:

Helen Johnston, Rob Fender, Kinwah Wu

Low Luminosity States of the Black Hole Candidate GX 339-4. I. ASCA and Simultaneous Radio/RXTE Observations

(1999)

Authors:

Joern Wilms, Michael Nowak, James B Dove, Robert P Fender, Tiziana Di Matteo

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