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Black Hole

Lensing of space time around a black hole. At Oxford we study black holes observationally and theoretically on all size and time scales - it is some of our core work.

Credit: ALAIN RIAZUELO, IAP/UPMC/CNRS. CLICK HERE TO VIEW MORE IMAGES.

Dr James Matthews

Royal Society University Research Fellow

Research theme

  • Astronomy and astrophysics
  • Particle astrophysics & cosmology

Sub department

  • Astrophysics

Research groups

  • Galaxy formation and evolution
  • MeerKAT
  • Pulsars, transients and relativistic astrophysics
  • Gamma-ray astronomy
james.matthews@physics.ox.ac.uk
Telephone: 01865(2)73299
Denys Wilkinson Building, room 763
Website
  • About
  • Into the Cosmos
  • Publications

The impact of accretion disc winds on the optical spectra of cataclysmic variables

Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) 450:3 (2015) 3331-3344

Authors:

JH Matthews, C Knigge, KS Long, SA Sim, N Higginbottom
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Details from ArXiV

LINE-DRIVEN DISK WINDS IN ACTIVE GALACTIC NUCLEI: THE CRITICAL IMPORTANCE OF IONIZATION AND RADIATIVE TRANSFER

The Astrophysical Journal American Astronomical Society 789:1 (2014) 19

Authors:

Nick Higginbottom, Daniel Proga, Christian Knigge, Knox S Long, James H Matthews, Stuart A Sim
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A simple disc wind model for broad absorption line quasars

Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) 436:2 (2013) 1390-1407

Authors:

N Higginbottom, C Knigge, KS Long, SA Sim, JH Matthews
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NEARBY PLANETARY SYSTEMS AS LENSES DURING PREDICTED CLOSE PASSAGES TO BACKGROUND STARS

The Astrophysical Journal American Astronomical Society 771:2 (2013) 79

Authors:

Rosanne Di Stefano, James Matthews, Sébastien Lépine
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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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