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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

Measuring the distance to the black hole candidate X-ray binary MAXI J1348-630 using HI absorption

(2020)

Authors:

J Chauhan, JCA Miller-Jones, W Raja, JR Allison, PFL Jacob, GE Anderson, F Carotenuto, S Corbel, R Fender, A Hotan, M Whiting, PA Woudt, B Koribalski, E Mahony

CHILES VERDES: Radio variability at an unprecedented depth and cadence in the COSMOS field

(2020)

Authors:

Sumit K Sarbadhicary, Evangelia Tremou, Adam J Stewart, Laura Chomiuk, Charee Peters, Chris Hales, Jay Strader, Emmanuel Momjian, Rob Fender, Eric M Wilcots

Rapid compact jet quenching in the Galactic black hole candidate X-ray binary MAXI J1535-571

(2020)

Authors:

TD Russell, M Lucchini, AJ Tetarenko, JCA Miller-Jones, GR Sivakoff, F Krau脽, W Mulaudzi, MC Baglio, DM Russell, D Altamirano, C Ceccobello, S Corbel, N Degenaar, J van den Eijnden, R Fender, S Heinz, KII Koljonen, D Maitra, S Markoff, S Migliari, AS Parikh, RM Plotkin, M Rupen, C Sarazin, R Soria, R Wijnands

Simultaneous multi-telescope observations of FRB 121102

Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) 496:4 (2020) 4565-4573

Authors:

M Caleb, BW Stappers, TD Abbott, ED Barr, MC Bezuidenhout, SJ Buchner, M Burgay, W Chen, I Cognard, LN Driessen, R Fender, GH Hilmarsson, J Hoang, DM Horn, F Jankowski, M Kramer, DR Lorimer, M Malenta, V Morello, M Pilia, E Platts, A Possenti, KM Rajwade, A Ridolfi, L Rhodes, S Sanidas, M Serylak, LG Spitler, LJ Townsend, A Weltman, PA Woudt, J Wu

Bow-shocks, nova shells, disc winds and tilted discs: The Nova-Like V341 Ara Has It All

(2020)

Authors:

N Castro Segura, C Knigge, JA Acosta-Pulido, D Altamirano, S del Palacio, JV Hernandez Santisteban, M Pahari, P Rodriguez-Gil, C Belardi, DAH Buckley, MR Burleigh, M Childress, RP Fender, DM Hewitt, DJ James, RB Kuhn, NPM Kuin, J Pepper, AA Ponomareva, ML Pretorius, JE Rodr铆guez, KG Stassun, DRA Williams, PA Woudt

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