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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.

Michele Cappellari

Professor of Astrophysics

Research theme

  • Astronomy and astrophysics

Sub department

  • Astrophysics

Research groups

  • Galaxy formation and evolution
  • Extremely Large Telescope
michele.cappellari@physics.ox.ac.uk
Telephone: 01865 (2)73647
Denys Wilkinson Building, room 755
  • About
  • Publications

The kinematics of Core and Cusp galaxies: comparing HST imaging and integral-field observations

(2007)

Authors:

J Falcón-Barroso, R Bacon, M Cappellari, RL Davies, PT de Zeeuw, E Emsellem, D Krajnovic, H Kuntschner, RM McDermid, RF Peletier, M Sarzi, G van de Ven
More details from the publisher

Towards a new classification of early-type galaxies: an integral-field view

(2007)

Authors:

J Falcón-Barroso, R Bacon, M Cappellari, RL Davies, PT de Zeeuw, E Emsellem, D Krajnovic, H Kuntschner, RM McDermid, RF Peletier, M Sarzi, G van de Ven
More details from the publisher

The SAURON project - IX. A kinematic classification for early-type galaxies

Monthly Notices of the Royal Astronomical Society 379 (2007) 401-417

Authors:

RL Davies, Eric Emsellem, Michele Cappellari, Davor Krajnovic
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The SAURON project - X. The orbital anisotropy of elliptical and lenticular galaxies: revisiting the (V/sigma,epsilon) diagram with integral-field stellar kinematics

Monthly Notices of the Royal Astronomical Society 379:2 (2007) 418-444

Authors:

M Cappellari, Bacon, R., Bureau, M., Emsellem, E.
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Revisiting the (V/sigma)-epsilon anisotropy diagram of early-type galaxies using integral-field kinematics

(2007)

Authors:

Michele Cappellari, R Bacon, Martin Bureau, RL Davies, PTD Zeeuw, E Emsellem, J Falcon-Barroso, D Krajnovic, H Kuntschner, RM McDermid, RF Peletier, M Sarzi, RCEVD Bosch, GVD Ven

Abstract:

We use integral-field observation of the stellar kinematics obtained with SAURON in combination with Schwarzschild dynamical models to revisit our understanding of the classic (V /σ) − ε anisotropy diagram of early-type galaxies.
Details from ORA
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