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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.

Professor Roger Davies

Emeritus Wetton Professor

Research theme

  • Astronomy and astrophysics
  • Instrumentation

Sub department

  • Astrophysics

Research groups

  • Astronomical instrumentation
  • Cosmology
  • Galaxy formation and evolution
  • Hintze Centre for Astrophysical Surveys
  • Rubin-LSST
  • Extremely Large Telescope
Roger.Davies@physics.ox.ac.uk
  • About
  • Publications

THE KINEMATIC PROPERTIES OF FAINT ELLIPTICAL GALAXIES

ASTROPHYSICAL JOURNAL 266:1 (1983) 41-57

Authors:

RL DAVIES, G EFSTATHIOU, SM FALL, G ILLINGWORTH, PL SCHECHTER
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A MASS ESTIMATE FOR THE COMPANION TO THE CARTWHEEL GALAXY

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 201:3 (1982) P69-&

Authors:

RL DAVIES, DC MORTON
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OBSERVATIONS OF THE DYNAMICS OF 8 EARLY-TYPE GALAXIES

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 194:3 (1981) 879-902
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THE METALLICITIES, VELOCITY DISPERSIONS AND TRUE SHAPES OF ELLIPTICAL GALAXIES

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 196:2 (1981) 381-395

Authors:

R TERLEVICH, RL DAVIES, SM FABER, D BURSTEIN
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Dynamical modeling of SAURON galaxies

Proceedings of IUTAM Symposia and Summer Schools IUTAM 3

Authors:

Michele Cappellari, RCEVD Bosch, EK Verolme, R Bacon, Martin Bureau, Y Copin, RL Davies, E Emsellem, D Krajnovic, H Kuntschner, R McDermid, BW Miller, RF Peletier, PTD Zeeuw

Abstract:

We describe our program for the dynamical modeling of early-type galaxies observed with the panoramic integral-field spectrograph SAURON. We are using Schwarzschild's numerical orbit superposition method to reproduce in detail all kinematical and photometric observables, and recover the intrinsic orbital structure of the galaxies. Since catastrophes are the most prominent features in the orbital observables, two-dimensional kinematical coverage is essential to constrain the dynamical models.

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