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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

Environment, Ram Pressure, and Shell Formation in Holmberg II

The Astronomical Journal 123 (2002) 1316-1333

Authors:

MG Bureau, C. Carignan
More details from the publisher

Probing the stellar populations of early-type galaxies: the SAURON survey

(2002)

Authors:

Eric Emsellem, Roger Davies, Richard McDermid, Harald Kuntschner, Reynier Peletier, Roland Bacon, Martin Bureau, Michele Cappellari, Yannick Copin, Bryan Miller, Ellen Verolme, Tim de Zeeuw
More details from the publisher

A SAURON study of M32: measuring the intrinsic flattening and the central black hole mass

(2002)

Authors:

EK Verolme, M Cappellari, Y Copin, RP van der Marel, R Bacon, M Bureau, RL Davies, BM Miller, PT de Zeeuw
More details from the publisher

A SAURON study of M32: measuring the intrinsic flattening and the central black hole mass

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 335:3 (2002) 517-525

Authors:

EK Verolme, M Cappellari, Y Copin, RP van der Marel, R Bacon, M Bureau, RL Davies, BM Miller, PT de Zeeuw
More details from the publisher

Probing the stellar populations of early-type galaxies: the SAURON survey

ASTR SOC P 282 (2002) 189-200

Authors:

E Emsellem, R Davies, R McDermid, H Kuntschner, R Peletier, R Bacon, M Bureau, M Cappellari, Y Copin, B Miller, E Verolme, T de Zeeuw

Abstract:

The SAURON project will deliver two-dimensional spectroscopic data of a sample of nearby early-type galaxies with unprecedented quality. In this paper, we focus on the mapping of their stellar populations using the SAURON data, and present some preliminary results on a few prototypical cases.
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