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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 prompt radio transient associated with a gamma-ray superflare from the young M dwarf binary DG CVn

Monthly Notices of the Royal Astronomical Society: Letters Oxford University Press (OUP) 446:1 (2015) l66-l70

Authors:

RP Fender, GE Anderson, R Osten, T Staley, C Rumsey, K Grainge, RDE Saunders
More details from the publisher
Details from ArXiV

Multi-wavelength studies of high-latitude black-Hole X-ray transients

Proceedings of Science 1-5-June-2015 (2015)

Authors:

PA Charles, AW Shaw, M Coriat, P Gandhi, LJ Townsend, P Woudt, J Casares, DL Foster, MM Kotze, D Steeghs, RP Fender, AA Zdziarski

Abstract:

Over the last 25 years ∼75% of the low-mass X-ray binary X-ray transients have been shown to contain black-hole compact objects, based on optical spectroscopy of their kinematics when in quiescence. Because many of these systems are extremely faint in quiescence and unobservable, we have utilised the method of studying them when in X-ray outburst that exploits the fluores- cence features produced by X-ray irradiation of the donor's inner face, thereby allowing us to track the motion of the donor. Such outbursts are unpredictable and hence these studies must necessarily be through Target-of-Opportunity programs, and hence are ideal for SALT for accessible targets. Here we report on our SALT ToO studies of two transients, both believed to contain black holes and both at high galactic latitude.

The truncated and evolving inner accretion disc of the black hole GX 339−4

Astronomy & Astrophysics EDP Sciences 573 (2015) a120

Authors:

DS Plant, RP Fender, G Ponti, T Muñoz-Darias, M Coriat
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LOFAR Observations of Swift J1644+57 and Implications for Short-Duration Transients

(2014)

Authors:

Y Cendes, RAMJ Wijers, JD Swinbank, A Rowlinson, AJ van der Horst, D Carbone, JW Broderick, TD Staley, AJ Stewart, G Molenaar, F Huizinga, A Alexov, ME Bell, T Coenen, S Corbel, J Eislöffel, R Fender, J Grießmeier, J Hessel, P Jonker, M Kramer, M Kuniyoshi, CJ Law, S Markoff, M Pietka, B Stappers, M Wise, P Zarka
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New methods to constrain the radio transient rate: results from a survey of four fields with LOFAR

(2014)

Authors:

D Carbone, AJ van der Horst, RAMJ Wijers, JD Swinbank, A Rowlinson, JW Broderick, YN Cendes, AJ Stewart, ME Bell, RP Breton, S Corbel, J Eislöffel, RP Fender, JM Grießmeier, JWT Hessels, PG Jonker, M Kramer, CJ Law, JCA Miller-Jones, M Pietka, LHA Scheers, BW Stappers, J van Leeuwen, R Wijnands, M Wise, P Zarka
More details from the publisher

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