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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.

Martin Bureau

Professor of Astrophysics

Research theme

  • Astronomy and astrophysics

Sub department

  • Astrophysics

Research groups

  • Galaxy formation and evolution
  • Hintze Centre for Astrophysical Surveys
martin.bureau@physics.ox.ac.uk
Telephone: 01865 (2)73377
Denys Wilkinson Building, room 701
Home page
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  • About
  • Publications

FCC 35 and Its H I Companion: Multiwavelength Observations and Interpretation

The Astronomical Journal American Astronomical Society 115:6 (1998) 2345-2355

Authors:

ME Putman, M Bureau, JR Mould, L Staveley-Smith, KC Freeman
More details from the publisher

The Nature of Boxy/Peanut Spiral Galaxies: Overview and New Results

Publications of the Astronomical Society of Australia Cambridge University Press (CUP) 14:2 (1997) 146-158

Authors:

M Bureau, KC Freeman
More details from the publisher

A New I-Band Tully-Fisher Relation for the Fornax Cluster: Implication for the Fornax Distance and Local Supercluster Velocity Field

The Astrophysical Journal American Astronomical Society 463 (1996) 60

Authors:

M Bureau, JR Mould, L Staveley-Smith
More details from the publisher

Dynamical Modeling of SAURON Galaxies

Carnegie Observatories Centennial Symposium. 1. Coevolution of Black Holes and Galaxies

Authors:

M Cappellari, RCE van den Bosch, EK Verolme, R Bacon, M Bureau, Y Copin, RL Davies, E Emsellem, D Krajnovic, H Kuntschner, R McDermid, BW Miller, RF Peletier, PT de 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.
Details from ORA
More details
Details from ArXiV

Neural Deprojection of Galaxy Stellar Mass Profiles

Machine Learning and the Physical Sciences Workshop, NeurIPS 2025

Authors:

MJ Yantovski-Barth, H Zhang, N Smyth, C Stone, Martin BUREAU, Y Hezaveh, L Perreault-Levasseur
Details from ORA

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