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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 hot and fast ultra-stripped supernova that likely formed a compact neutron star binary

Science American Association for the Advancement of Science 362:6411 (2018) 201-206

Authors:

K De, MM Kasliwal, EO Ofek, TJ Moriya, J Burke, Y Cao, SB Cenko, GB Doran, GE Duggan, Robert Fender, C Fransson, A Gal-Yam, A Horesh, Kulkarni, RR Laher, R Lunnan, I Manulis, F Masci, PA Mazzali, PE Nugent, DA Perley, T Petrushevska, AL Piro, C Rumsey, J Sollerman, M Sullivan, F Taddia

Abstract:

Compact neutron star binary systems are produced from binary massive stars through stellar evolution involving up to two supernova explosions. The final stages in the formation of these systems have not been directly observed. We report the discovery of iPTF 14gqr (SN 2014ft), a type Ic supernova with a fast-evolving light curve indicating an extremely low ejecta mass (≈0.2 solar masses) and low kinetic energy (≈2 × 1050 ergs). Early photometry and spectroscopy reveal evidence of shock cooling of an extended helium-rich envelope, likely ejected in an intense pre-explosion mass-loss episode of the progenitor. Taken together, we interpret iPTF 14gqr as evidence for ultra-stripped supernovae that form neutron stars in compact binary systems.
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Tracking the variable jets of V404 Cygni during its 2015 outburst

(2018)

Authors:

AJ Tetarenko, GR Sivakoff, JCA Miller-Jones, M Bremer, KP Mooley, RP Fender, C Rumsey, A Bahramian, D Altamirano, S Heinz, D Maitra, SB Markoff, S Migliari, MP Rupen, DM Russell, TD Russell, CL Sarazin
More details from the publisher

A hot and fast ultra-stripped supernova that likely formed a compact neutron star binary

(2018)

Authors:

K De, MM Kasliwal, EO Ofek, TJ Moriya, J Burke, Y Cao, SB Cenko, GB Doran, GE Duggan, RP Fender, C Fransson, A Gal-Yam, A Horesh, SR Kulkarni, RR Laher, R Lunnan, I Manulis, F Masci, PA Mazzali, PE Nugent, DA Perley, T Petrushevska, AL Piro, C Rumsey, J Sollerman, M Sullivan, F Taddia
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The first tidal disruption flare in ZTF: from photometric selection to multi-wavelength characterization

(2018)

Authors:

Sjoert van Velzen, Suvi Gezari, S Bradley Cenko, Erin Kara, James C Miller-Jones, Tiara Hung, Joe Bright, Nathaniel Roth, Nadejda Blagorodnova, Daniela Huppenkothen, Lin Yan, Eran Ofek, Jesper Sollerman, Sara Frederick, Charlotte Ward, Matthew J Graham, Rob Fender, Mansi M Kasliwal, Chris Canella, Robert Stein, Matteo Giomi, Valery Brinnel, Jakob Santen, Jakob Nordin, Eric C Bellm, Richard Dekany, Christoffer Fremling, V Zach Golkhou, Thomas Kupfer, Shrinivas R Kulkarni, Russ R Laher, Ashish Mahabal, Frank J Masci, Adam A Miller, James D Neill, Reed Riddle, Mickael Rigault, Ben Rusholme, Maayane T Soumagnac, Yutaro Tachibana
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Identifying transient and variable sources in radio images

(2018)

Authors:

Antonia Rowlinson, Adam J Stewart, Jess W Broderick, John D Swinbank, Ralph AMJ Wijers, Dario Carbone, Yvette Cendes, Rob Fender, Alexander van der Horst, Gijs Molenaar, Bart Scheers, Tim Staley, Sean Farrell, Jean-Mathias Grießmeier, Martin Bell, Jochen Eislöffel, Casey J Law, Joeri van Leeuwen, Philippe Zarka
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