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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

Rapid Infrared Flares in Cygnus X-3

Chapter in Frontiers of Space And Ground-Based Astronomy, Springer Nature 187 (1994) 615-616

Authors:

RP Fender, SJ Bell Burnell
More details from the publisher

A persistent ultraviolet outflow from the accretion disc in a transient neutron star binary

Authors:

Noel Castro Segura, Christian Knigge, Knox Long, Diego Altamirano, Montserrat Armas Padilla, Charles Bailyn, David Buckley, Douglas Buisson, Jorge Casares, Phil Charles, Jorge Combi, Virginia A Cúneo, Nathalie Degenaar, Santiago del Palacio, Maria Diaz Trigo, Rob Fender, Poshak Gandhi, Claudia Gutíerrez, Juan Hernández Santisteban, Felipe Jiménez Ibarra, James Matthews, Mariano Mendez, Matthew Middleton, Teo Muñoz Darias, Mehtap Özbey Arabaci, Mayukh Pahari, Lauren Rhodes, Thomas Russell, Simone Scaringi, Jakob van den Eijden, Georgios Vasilopolulos, Federico Vincentelli, Phil Wiseman
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The 2018 outburst of BHXB H1743-322 as seen with MeerKAT

Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP)

Authors:

DRA Williams, SE Motta, R Fender, J Bright, I Heywood, E Tremou, P Woudt, DAH Buckley, S Corbel, M Coriat, T Joseph, L Rhodes, GR Sivakoff, AJ van der Horst

Abstract:

In recent years, the black hole candidate X-ray binary system H1743-322 has undergone outbursts and it has been observed with X-ray and radio telescopes. We present 1.3 GHz MeerKAT radio data from the ThunderKAT Large Survey Project on radio transients for the 2018 outburst of H1743-322. We obtain seven detections from a weekly monitoring programme and use publicly available Swift X-ray Telescope and MAXI data to investigate the radio/X-ray correlation of H1743-322 for this outburst. We compare the 2018 outburst with those reported in the literature for this system and find that the X-ray outburst reported is similar to previously reported `hard-only' outbursts. As in previous outbursts, H1743-322 follows the `radio-quiet' correlation in the radio/X-ray plane for black hole X-ray binaries, and the radio spectral index throughout the outburst is consistent with the `radio-quiet' population.
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The Birth of a Relativistic Jet Following the Disruption of a Star by a Cosmological Black Hole

Authors:

Dheeraj Pasham, Matteo Lucchini, Tanmoy Laskar, Benjamin Gompertz, Shubham Srivas, Matt Nicholl, Stephen Smartt, James Miller-Jones, Kate Alexander, Rob Fender, Graham Smith, Michael Fulton, Gulab Dewangan, Keith Gendreau, Lauren Rhodes, Assaf Horesh, Sjoert van Velzen, Itai Sfaradi, Muryel Guolo, N Castro Segura, Aysha Aamer, Joseph Anderson, Iair Arcavi, Seán Brennan, Kenneth Chambers, Panos Charalampopoulos, Ting-Wan Chen, Alejandro Clocchiatti, Thomas de Boer, Michel Dennefeld, Elizabeth Ferrara, Lluís Galbany, Hua Gao, James Gillanders, Adelle Goodwin, Mariusz Gromadzki, M Huber, Peter Jonker, Manasvita Joshi, Erin Kara, Thomas Killestein, Peter Kosec, Daniel Kocevski, Giorgos Leloudas, Chien-Cheng Lin, Raffaella Margutti, Seppo Mattila, Thomas Moore, Tom ’as M\”uller-Bravo, Chow-Choong Ngeow, Samantha Oates, Francesca Onori, Yen-Chen Pan, Miguel Perez Torres, Priyanka Rani, Ronald Remillard, E Ridley, Steve Schulze, Xinyue Sheng, Luke Shingles, Ken Smith, James Steiner, Richard Wainscoat, Thomas Wevers, Sheng Yang
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Details from ArXiV

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