Gamma-ray astronomy

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Simultaneous millimetre and radio observations of Cygnus X-3 in a quiescent radio state

Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) 274:2 (1995) 633-638

Authors:

RP Fender, SJ Bell Burnell, ST Garrington, RE Spencer, GG Pooley
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8C1435+635 - A RADIO GALAXY AT Z=4.25

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 271:2 (1994) 504-512

Authors:

M LACY, G MILEY, S RAWLINGS, R SAUNDERS, M DICKINSON, S GARRINGTON, S MADDOX, G POOLEY, CC STEIDEL, MN BREMER, G COTTER, R VANOJIK, H ROTTGERING, P WARNER
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Rapid Infrared Flares in Cygnus X-3

Chapter in Frontiers of Space And Ground-Based Astronomy, Springer Nature 187 (1994) 615-616

Authors:

RP Fender, SJ Bell Burnell
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A persistent ultraviolet outflow from the accretion disc in a transient neutron star binary

Authors:

Noel Castro Segura, Christian Knigge, Knox Long, Diego Altamirano, Montserrat Armas Padilla, Charles Bailyn, David Buckley, Douglas Buisson, Jorge Casares, Phil Charles, Jorge Combi, Virginia A Cúneo, Nathalie Degenaar, Santiago del Palacio, Maria Diaz Trigo, Rob Fender, Poshak Gandhi, Claudia Gutíerrez, Juan Hernández Santisteban, Felipe Jiménez Ibarra, James Matthews, Mariano Mendez, Matthew Middleton, Teo Muñoz Darias, Mehtap Özbey Arabaci, Mayukh Pahari, Lauren Rhodes, Thomas Russell, Simone Scaringi, Jakob van den Eijden, Georgios Vasilopolulos, Federico Vincentelli, Phil Wiseman
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Fornax A, Centaurus A and other radio galaxies as sources of ultra-high energy cosmic rays

Monthly Notices of the Royal Astronomical Society: Letters Blackwell Publishing

Authors:

JH Matthews, AR Bell, KM Blundell, AT Araudo

Abstract:

The origin of ultra-high energy cosmic rays (UHECRs) is still unknown. It has recently been proposed that UHECR anisotropies can be attributed to starbust galaxies or active galactic nuclei. We suggest that the latter is more likely and that giant-lobed radio galaxies such as Centaurus A and Fornax A can explain the data.
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