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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

Powerful jets from black hole X-ray binaries in Low/Hard X-ray states

(2000)
More details from the publisher

The infrared counterpart of the Z source GX 5-1

Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) 315:4 (2000) l57-l60

Authors:

PG Jonker, RP Fender, NC Hambly, M van der Klis
More details from the publisher

Giant repeated ejections from GRS 1915+105

(2000)

Authors:

RP Fender, GG Pooley
More details from the publisher

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

(2000)

Authors:

SGH Berendsen, R Fender, E Kuulkers, J Heise, M van der Klis
More details from the publisher

ASTRONOMY: A New Source of Gamma Rays.

Science (New York, N.Y.) 288:5475 (2000) 2326

Abstract:

Relativistic outflows or "jets" are collimated streams of high-energy electrons that emit synchrotron radiation at radio wavelengths and have bulk velocities that are a substantial fraction of the speed of light. They trace the outflow of enormous amounts of energy and matter from a central supermassive black hole in distant radio galaxies. As Fender explains in this Perspective, much smaller, more local sources may also produce such jets. Data presented by Paredes et al. point toward association of one such source, a relatively faint x-ray binary, with a gamma-ray source. This and similar pairs may contribute substantially to the production of high-energy particles and photons within our galaxy.
More details from the publisher
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