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.

Multiwavelength Observations of GX 339–4 in 1996. I. Daily Light Curves and X-Ray and Gamma-Ray Spectroscopy

The Astrophysical Journal American Astronomical Society 519:2 (1999) 762-770

Authors:

IA Smith, EP Liang, D Lin, M Moss, A Crider, RP Fender, Ph Durouchoux, S Corbel, R Sood

Quenching of the Radio Jet during the X-Ray High State of GX 339–4

The Astrophysical Journal American Astronomical Society 519:2 (1999) l165-l168

Authors:

Robert Fender, Stéphane Corbel, Tasso Tzioumis, Vince McIntyre, Duncan Campbell-Wilson, Mike Nowak, Ravi Sood, Richard Hunstead, Alan Harmon, Philippe Durouchoux, William Heindl

The Bulge-Disk Orthogonal Decoupling in Galaxies: NGC 4698**Based on observations carried out at ESO, La Silla, Chile (ESO N. 60.A-0800).

The Astrophysical Journal American Astronomical Society 519:2 (1999) l127-l130

Authors:

F Bertola, EM Corsini, JC Vega Beltrán, A Pizzella, M Sarzi, M Cappellari, SJJG Funes

On the nature of XTE J0421+560/CI Cam

(1999)

Authors:

T Belloni, S Dieters, ME van den Ancker, RP Fender, DW Fox, BA Harmon, M van der Klis, JM Kommers, WHG Lewin, J van Paradijs

Relativistic Jets from X-ray binaries

(1999)

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