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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 parsec scale X-ray extended structure from the X-ray binary Circinus X-1

Monthly Notices of the Royal Astronomical Society Letters 397:1 (2009) L1-L5

Authors:

P Soleri, S Heinz, R Fender, R Wijnands, V Tudose, D Altamirano, PG Jonker, M van der Kris, L Kuiper, C Kaiser, P Casella

Abstract:

We present the results of the analysis of two Chandra observations of Circinus X-1 performed in 2007, for a total exposure time of ~50 ks. The source was observed with the High Resolution Camera during a long X-ray low-flux state of the source. Cir X-1 is an accreting neutron star binary system that exhibits ultra-relativistic arcsec-scale radio jets and an extended arcmin-scale radio nebula. Furthermore, a recent paper has shown an X-ray excess on arcmin-scale prominent on the side of the receding radio jet. In our images, we clearly detect X-ray structures on both the side of the receding and the approaching radio jet. The X-ray emission is consistent with a synchrotron origin. Our detection is consistent with neutron star binaries being as efficient as black hole binaries in producing X-ray outflows, despite their shallower gravitational potential. 漏 2009 The Authors. Journal compilation 漏 2009 RAS.

Linking jet emission and X-ray properties in the peculiar neutron star X-ray binary Circinus X-1

(2009)

Authors:

Paolo Soleri, Valeriu Tudose, Rob Fender, Michiel van der Klis, Peter G Jonker

A global study of X-ray binaries

Sissa Medialab Srl (2009) 008

Authors:

Robert Dunn, Rob Fender, Elmar K枚rding, Clement Cabanac, Tomaso Belloni

Internal Shocks Model for Microquasar Jets

Sissa Medialab Srl (2009) 026

Authors:

Omar Jamil, Rob Fender, Christian R Kaiser

Monitoring LMXBs with the Faulkes Telescope

Sissa Medialab Srl (2009) 069

Authors:

Fraser Lewis, David M Russell, Rob Fender, Paul Roche, J Simon Clark

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