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.

The XMM-Newton/Chandra monitoring campaign of the Galactic center region

Astronomy & Astrophysics EDP Sciences 449:3 (2006) 1117-1127

Authors:

R Wijnands, JJM in 't Zand, M Rupen, T Maccarone, J Homan, R Cornelisse, R Fender, J Grindlay, M van der Klis, E Kuulkers, CB Markwardt, JCA Miller-Jones, QD Wang

Jet-dominated advective systems: radio and X-ray luminosity dependence on the accretion rate

(2006)

Authors:

Elmar Koerding, Rob Fender, Simone Migliari

A ULX microquasar in NGC 5408?

(2006)

Authors:

Roberto Soria, Rob Fender, Diana Hannikainen, Andrew Read, Ian Stevens

Structure in the radio counterpart to the 2004 December 27 giant flare from SGR 1806–20

Monthly Notices of the Royal Astronomical Society: Letters Oxford University Press (OUP) 367:1 (2006) l6-l10

Authors:

RP Fender, TWB Muxlow, MA Garrett, C Kouveliotou, BM Gaensler, ST Garrington, Z Paragi, V Tudose, JCA Miller-Jones, RE Spencer, RAM Wijers, GB Taylor

A transient relativistic radio jet from Cygnus X-1

(2006)

Authors:

RP Fender, AM Stirling, RE Spencer, I Brown, GG Pooley, TWB Muxlow, JCA Miller-Jones

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