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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

A highly polarised radio jet during the 1998 outburst of the black hole transient XTE J1748-288

(2007)

Authors:

Catherine Brocksopp, James Miller-Jones, Rob Fender, Ben Stappers
More details from the publisher

The jet-powered optical nebula of Cygnus X–1

Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) 376:3 (2007) 1341-1349

Authors:

DM Russell, RP Fender, E Gallo, CR Kaiser
More details from the publisher
Details from ArXiV

Peak Luminosities of the Hard States of GX 339-4: Implications for the Accretion Geometry, Disk Mass, and Black Hole Mass

(2007)

Authors:

Wenfei Yu, Frederick K Lamb, Robert Fender, Michiel van der Klis
More details from the publisher

Evidence for deceleration in the radio jets of GRS 1915+105?

Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) 375:3 (2007) 1087-1098

Authors:

JCA Miller-Jones, MP Rupen, RP Fender, A Rushton, GG Pooley, RE Spencer
More details from the publisher
Details from ArXiV

Rossi X-Ray Timing Explorer Observations of the First Transient Z Source XTE J1701–462: Shedding New Light on Mass Accretion in Luminous Neutron Star X-Ray Binaries

The Astrophysical Journal American Astronomical Society 656:1 (2007) 420-430

Authors:

Jeroen Homan, Michiel van der Klis, Rudy Wijnands, Tomaso Belloni, Rob Fender, Marc Klein-Wolt, Piergiorgio Casella, Mariano Méndez, Elena Gallo, Walter HG Lewin, Neil Gehrels
More details from the publisher

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