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.

A connection between accretion state and Fe K absorption in an accreting neutron star: black hole-like soft-state winds?

Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) 444:2 (2014) 1829-1834

Authors:

Gabriele Ponti, Teodoro Muñoz-Darias, Robert P Fender

Engulfing a radio pulsar: the case of PSR J1023+0038

Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) 444:2 (2014) 1783-1792

Authors:

F Coti Zelati, MC Baglio, S Campana, P D'Avanzo, P Goldoni, N Masetti, T Muñoz-Darias, S Covino, RP Fender, E Jiménez Bailón, H Otí-Floranes, E Palazzi, FG Ramón-Fox

Swift J1357.2−0933: the faintest black hole?

Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) 444:1 (2014) 902-905

Authors:

M Armas Padilla, R Wijnands, N Degenaar, T Muñoz-Darias, J Casares, RP Fender

A prompt radio transient associated with a gamma-ray superflare from the young M dwarf binary DG CVn

(2014)

Authors:

RP Fender, GE Anderson, R Osten, T Staley, C Rumsey, K Grainge, RDE Saunders

Black hole-like hysteresis and accretion states in neutron star low-mass X-ray binaries

Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) 443:4 (2014) 3270-3283

Authors:

T Muñoz-Darias, RP Fender, SE Motta, TM Belloni

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