Skip to main content
Home
Department Of Physics text logo
  • Research
    • Our research
    • Our research groups
    • Our research in action
    • Research funding support
    • Summer internships for undergraduates
  • Study
    • Undergraduates
    • Postgraduates
  • Engage
    • For alumni
    • For business
    • For schools
    • For the public
Menu
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 spectroscopic, photometric, polarimetric and radio study of the eclipsing polar UZ Fornacis: the first simultaneous SALT and MeerKAT observations

(2020)

Authors:

Zwidofhelangani N Khangale, Stephen B Potter, Patrick A Woudt, David AH Buckley, Andrey N Semena, Enrico J Kotze, Danièl N Groenewald, Dante M Hewitt, Margaretha L Pretorius, Rob P Fender, Paul Groot, Steven Bloemen, Marc Klein-Wolt, Elmar Körding, Rudolf Le Poole, Vanessa A McBride, Lee Townsend, Kerry Paterson, Danielle LA Pieterse, Paul M Vreeswijk
More details from the publisher

MKT J170456.2-482100: the first transient discovered by MeerKAT

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 491:1 (2020) 560-575

Authors:

Ln Driessen, I McDonald, Dah Buckley, M Caleb, Ej Kotze, Sb Potter, Km Rajwade, A Rowlinson, Bw Stappers, E Tremou, Pa Woudt, Rp Fender, R Armstrong, P Groot, I Heywood, A Horesh, Aj van der Horst, E Koerding, Va McBride, Jca Miller-Jones, Kp Mooley, Ramj Wijers

Abstract:

© 2019 The Author(s) We report the discovery of the first transient with MeerKAT, MKT J170456.2−482100, discovered in ThunderKAT images of the low-mass X-ray binary GX339−4. MKT J170456.2−482100 is variable in the radio, reaching a maximum flux density of 0.71 ± 0.11 mJy on 2019 October 12, and is undetected in 15 out of 48 ThunderKAT epochs. MKT J170456.2−482100 is coincident with the chromospherically active K-type sub-giant TYC 8332-2529-1, and ∼ 18 yr of archival optical photometry of the star shows that it varies with a period of 21.25 ± 0.04 d. The shape and phase of the optical light curve changes over time, and we detect both X-ray and UV emission at the position of MKT J170456.2−482100, which may indicate that TYC 8332-2529-1 has large star spots. Spectroscopic analysis shows that TYC 8332-2529-1 is in a binary, and has a line-of-sight radial velocity amplitude of 43 km s−1. We also observe a spectral feature in antiphase with the K-type sub-giant, with a line-of-sight radial velocity amplitude of ∼ 12 ± 10 km s−1, whose origins cannot currently be explained. Further observations and investigation are required to determine the nature of the MKT J170456.2−482100 system.
More details from the publisher
Details from ORA
More details
Details from ArXiV

Evidence for Late-stage Eruptive Mass Loss in the Progenitor to SN2018gep, a Broad-lined Ic Supernova: Pre-explosion Emission and a Rapidly Rising Luminous Transient

The Astrophysical Journal American Astronomical Society 887:2 (2019) 169

Authors:

Anna YQ Ho, Daniel A Goldstein, Steve Schulze, David K Khatami, Daniel A Perley, Mattias Ergon, Avishay Gal-Yam, Alessandra Corsi, Igor Andreoni, Cristina Barbarino, Eric C Bellm, Nadia Blagorodnova, Joe S Bright, E Burns, S Bradley Cenko, Virginia Cunningham, Kishalay De, Richard Dekany, Alison Dugas, Rob P Fender, Claes Fransson, Christoffer Fremling, Adam Goldstein, Matthew J Graham, David Hale, Assaf Horesh, Tiara Hung, Mansi M Kasliwal, N Paul M Kuin, SR Kulkarni, Thomas Kupfer, Ragnhild Lunnan, Frank J Masci, Chow-Choong Ngeow, Peter E Nugent, Eran O Ofek, Maria T Patterson, Glen Petitpas, Ben Rusholme, Hanna Sai, Itai Sfaradi, David L Shupe, Jesper Sollerman, Maayane T Soumagnac, Yutaro Tachibana, Francesco Taddia, Richard Walters, Xiaofeng Wang, Yuhan Yao, Xinhan Zhang
More details from the publisher

A radio parallax to the black hole X-ray binary MAXI J1820+070

(2019)

Authors:

P Atri, JCA Miller-Jones, A Bahramian, RM Plotkin, AT Deller, PG Jonker, TJ Maccarone, GR Sivakoff, R Soria, D Altamirano, T Belloni, R Fender, E Koerding, D Maitra, S Markoff, S Migliari, D Russell, T Russell, CL Sarazin, AJ Tetarenko, V Tudose
More details from the publisher

Physical Constraints from Near-infrared Fast Photometry of the Black Hole Transient GX 339–4

The Astrophysical Journal Letters American Astronomical Society 887:1 (2019) l19

Authors:

FM Vincentelli, P Casella, P Petrucci, T Maccarone, DM Russell, P Uttley, B De Marco, R Fender, P Gandhi, J Malzac, K O’Brien, JA Tomsick
More details from the publisher
More details

Pagination

  • First page First
  • Previous page Prev
  • …
  • Page 39
  • Page 40
  • Page 41
  • Page 42
  • Current page 43
  • Page 44
  • Page 45
  • Page 46
  • Page 47
  • …
  • Next page Next
  • Last page Last

Footer Menu

  • Contact us
  • Giving to the Dept of Physics
  • Work with us
  • Media

User account menu

  • Log in

Follow us

FIND US

Clarendon Laboratory,

Parks Road,

Oxford,

OX1 3PU

CONTACT US

Tel: +44(0)1865272200

University of Oxfrod logo Department Of Physics text logo
IOP Juno Champion logo Athena Swan Silver Award logo

© University of Oxford - Department of Physics

Cookies | Privacy policy | Accessibility statement

Built by: Versantus

  • Home
  • Research
  • Study
  • Engage
  • Our people
  • News & Comment
  • Events
  • Our facilities & services
  • About us
  • Current students
  • Staff intranet