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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

Simultaneous radio and X-ray observations of Galactic Centre low-mass X-ray binaries

Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) 318:2 (2000) 599-605

Authors:

Stephan GH Berendsen, Robert Fender, Erik Kuulkers, J Heise, M van der Klis
More details from the publisher

Giant repeated ejections from GRS 1915+105

Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) 318:1 (2000) l1-l5

Authors:

RP Fender, GG Pooley
More details from the publisher

Orbital Dynamics of Cygnus X-3

The Astrophysical Journal American Astronomical Society 541:1 (2000) 308-318

Authors:

MM Hanson, MD Still, RP Fender
More details from the publisher

Excess submillimetre emission from GRS 1915+105

Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) 317:1 (2000) 158-162

Authors:

RN Ogley, SJ Bell Burnell, RP Fender, GG Pooley, EB Waltman
More details from the publisher

The radio luminosity of persistent X-ray binaries

Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) 317:1 (2000) 1-8

Authors:

RP Fender, MA Hendry
More details from the publisher

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