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.

Disc-jet coupling in an atoll-type neutron star X-ray binary: 4U 1728-34 (GX 354-0)

(2003)

Authors:

Simone Migliari, Rob Fender, Michael Rupen, Peter Jonker, Marc Klein-Wolt, Robert Hjellming, Michiel van der Klis

Peculiar spectral and power spectral behaviour of the LMXB GX 13+1

(2003)

Authors:

RS Schnerr, T Reerink, M van der Klis, J Homan, M Méndez, RP Fender, E Kuulkers

Uses and limitations of relativistic jet proper motions: lessons from Galactic microquasars

Monthly Notices of the Royal Astronomical Society 91̽�� University Press (OUP) 340:4 (2003) 1353-1358

Hard X-ray Flares Preceding Soft X-ray Outbursts in Aquila X-1: A Link between Neutron Star and Black Hole State Transitions

(2003)

Authors:

Wenfei Yu, Marc Klein-Wolt, Rob Fender, Michiel van der Klis

The mass of the neutron star in Vela X-1 and tidally induced non-radial oscillations in GP Vel

Astronomy & Astrophysics EDP Sciences 401:1 (2003) 313-323

Authors:

H Quaintrell, AJ Norton, TDC Ash, P Roche, B Willems, TR Bedding, IK Baldry, RP Fender

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