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19962009
most citedGlobal optical/infrared - X-ray correlations in X-ray binaries: quantifying disc and jet contributions

245 citations · 1.9k across the 46 of their papers we have counts for

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Showing 2005Show all

8 papers · 1 filter

astro-ph20051 cited

Accretion modes and jet production in black hole X-ray binaries

Elena Gallo, Rob Fender

We review our current understanding of the radio properties of black hole X-ray binaries in connection with the X-ray spectral states, and discuss them in the framework of the rece…

astro-ph2005

Multiple relativistic outbursts of GRS 1915+105: radio emission and internal shocks

J. C. A. Miller-Jones, D. G. McCormick, R. P. Fender +3

We present 5-GHz MERLIN radio images of the microquasar GRS 1915+105 during two separate outbursts in 2001 March and 2001 July, following the evolution of the jet components as the…

astro-ph2005

A dark jet dominates the power output of the stellar black hole Cygnus X-1

E. Gallo, R. Fender, C. Kaiser +4

Accreting black holes are thought to emit the bulk of their power in the X-ray band by releasing the gravitational potential energy of the infalling matter. At the same time, they…

astro-ph2005

A unified model for black hole X-ray binary jets ?

Rob Fender, Tomaso Belloni, Elena Gallo

We have recently put forward a 'unified' semi-empirical model for the coupling between accretion and jet production in galactic black hole X-ray binaries (published in MNRAS, 2004)…

astro-ph2005

Energisation of interstellar media and cosmic ray production by jets from X-ray binaries

Rob Fender, Tom Maccarone, Zdenko van Kesteren

Drawing on recent estimates of the power of jets from X-ray binary systems as a function of X-ray luminosity, combined with improved estimates of the relevant Log(N)-Log(L_X) lumin…

astro-ph2005

The Growth, Polarization, and Motion of the Radio Afterglow from the Giant Flare from SGR 1806-20

G. B. Taylor, J. D. Gelfand, B. M. Gaensler +8

The extraordinary giant flare (GF) of 2004 December 27 from the soft gamma repeater (SGR) 1806-20 was followed by a bright radio afterglow. We present an analysis of VLA observatio…