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.

Was the Narrow Line Seyfert 1 RGB J0044+193 ever radio loud?

Astronomy & Astrophysics EDP Sciences 433:2 (2005) 531-533

Authors:

TJ Maccarone, JCA Miller-Jones, RP Fender, GG Pooley

An expanding radio nebula produced by a giant flare from the magnetar SGR 1806-20

(2005)

Authors:

BM Gaensler, C Kouveliotou, JD Gelfand, GB Taylor, D Eichler, RAMJ Wijers, J Granot, E Ramirez-Ruiz, YE Lyubarsky, RW Hunstead, D Campbell-Wilson, AJ van der Host, MA McLaughlin, RP Fender, MA Garrett, KJ Newton-McGee, DM Palmer, N Gehrels, PM Woods

On the Soft Excess in the X-Ray Spectrum of Circinus X-1: Revisitation of the Distance to Circinus X-1

The Astrophysical Journal American Astronomical Society 619:1 (2005) 503-516

Authors:

R Iaria, M Spanò, T Di Salvo, NR Robba, L Burderi, R Fender, M van der Klis, F Frontera

Black hole X-ray binary jets

(2005)

Authors:

Elena Gallo, Rob Fender, Christian Kaiser

Rapid variability of the arcsec-scale X-ray jets of SS 433

(2005)

Authors:

S Migliari, RP Fender, KM Blundell, M Mendez, M van der Klis

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