Professor Rob Fender: Publications

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.

Filling the radio transients gap

Astronomy & Geophysics Oxford University Press (OUP) 64:6 (2023) 6.24-6.30

Authors:

R Fender, A Horesh, P Charles, P Woudt, J Miller-Jones, J Bright

Fast infrared winds during the radio-loud and X-ray obscured stages of the black hole transient GRS 1915+105

Astronomy & Astrophysics EDP Sciences 680 (2023) l16

Authors:

J Sánchez-Sierras, T Muñoz-Darias, SE Motta, RP Fender, A Bahramian, C Martínez-Sebastián, JA Fernández-Ontiveros, J Casares, M Armas Padilla, DA Green, D Mata Sánchez, J Strader, MAP Torres

The dense and non-homogeneous circumstellar medium revealed in radio wavelengths around the Type Ib SN 2019oys

(2023)

Authors:

Itai Sfaradi, Assaf Horesh, Jesper Sollerman, Rob Fender, Lauren Rhodes, David RA Williams, Joe Bright, Dave A Green, Steve Schulze, Avishay Gal-Yam

An off-axis relativistic jet seen in the long lasting delayed radio flare of the TDE AT 2018hyz

Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) 527:3 (2023) 7672-7680

Authors:

Itai Sfaradi, Paz Beniamini, Assaf Horesh, Tsvi Piran, Joe Bright, Lauren Rhodes, David RA Williams, Rob Fender, James K Leung, Tara Murphy, Dave A Green

SAX J1810.8-2609: An Outbursting Neutron Star X-ray Binary with Persistent Spatially Coincident Radio Emission

(2023)

Authors:

AK Hughes, GR Sivakoff, J van den Eijnden, R Fender, JCA Miller-Jones, E Tremou

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