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.

A LINK BETWEEN X-RAY EMISSION LINES AND RADIO JETS IN 4U 1630–47?

The Astrophysical Journal Letters American Astronomical Society 784:1 (2014) l5

Authors:

Joseph Neilsen, Mickaël Coriat, Rob Fender, Julia C Lee, Gabriele Ponti, Anastasios K Tzioumis, Philip G Edwards, Jess W Broderick

Probing the Bright Radio Flare and Afterglow of GRB 130427A with the Arcminute Microkelvin Imager

(2014)

Authors:

GE Anderson, AJ van der Horst, TD Staley, RP Fender, RAMJ Wijers, AMM Scaife, C Rumsey, DJ Titterington, A Rowlinson, RDE Saunders

A Link Between X-ray Emission Lines and Radio Jets in 4U 1630-47?

(2014)

Authors:

Joseph Neilsen, Mickael Coriat, Rob Fender, Julia C Lee, Gabriele Ponti, Tasso Tzioumis, Phil Edwards, Jess W Broderick

Observational characteristics of accretion onto black holes II: environment and feedback

Cambridge University Press (CUP) (2014) 227-252

Discovery of Carbon Radio Recombination Lines in absorption towards Cygnus~A

(2014)

Authors:

JBR Oonk, RJ van Weeren, F Salgado, LK Morabito, AGGM Tielens, HJA Rottgering, A Asgekar, GJ White, A Alexov, J Anderson, IM Avruch, F Batejat, R Beck, ME Bell, I van Bemmel, MJ Bentum, G Bernardi, P Best, A Bonafede, F Breitling, M Brentjens, J Broderick, M Brueggen, HR Butcher, B Ciardi, JE Conway, A Corstanje, F de Gasperin, E de Geus, M de Vos, S Duscha, J Eisloeffel, D Engels, J van Enst, H Falcke, RA Fallows, R Fender, C Ferrari, W Frieswijk, MA Garrett, J Griessmeier, JP Hamaker, TE Hassall, G Heald, JWT Hessels, M Hoeft, A Horneffer, A van der Horst, M Iacobelli, NJ Jackson, E Juette, A Karastergiou, W Klijn, J Kohler, VI Kondratiev, M Kramer, M Kuniyoshi, G Kuper, J van Leeuwen, P Maat, G Macario, G Mann, S Markoff, JP McKean, M Mevius, JCA Miller-Jones, JD Mol, DD Mulcahy, H Munk, MJ Norden, E Orru, H Paas, M Pandey-Pommier, VN Pandey, R Pizzo, AG Polatidis, W Reich, AMM Scaife, A Schoenmakers, D Schwarz, A Shulevski, J Sluman, O Smirnov, C Sobey, BW Stappers, M Steinmetz, J Swinbank, M Tagger, Y Tang, C Tasse, S ter Veen, S Thoudam, C Toribio, R van Nieuwpoort, R Vermeulen, C Vocks, C Vogt, RAMJ Wijers, MW Wise, O Wucknitz, S Yatawatta, P Zarka, A Zensus

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