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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

Circumnuclear Keplerian Disks in Galaxies

(1998)

Authors:

F Bertola, M Cappellari, JG Funes, EM Corsini, A Pizzella, JC Vega Beltran
More details from the publisher

The Mini AGN at the Center of the Elliptical Galaxy NGC 4552 with HST

(1998)

Authors:

Michele Cappellari, Alvio Renzini, Laura Greggio, Sperello di Serego Alighieri, Lucio M Buson, David Burstein, Francesco Bertola
More details from the publisher

Circumnuclear Keplerian disks in galaxies

ASTROPHYSICAL JOURNAL 509:2 (1998) L93-L96

Authors:

F Bertola, M Cappellari, JG Funes, EM Corsini, A Pizzella, JCV Beltrán
More details from the publisher

UV imaging of the galaxy cluster CL0939+72 at z similar to 0.4

ASTR SOC P 146 (1998) 488-491

Authors:

LM Buson, F Bertola, M Cappellari, C Chiosi, A Dressler, A Oemler
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The variable UV central spike of NGC 4552

ASTR SOC P 117 (1997) 545-549

Authors:

M Cappellari, D Burstein, LM Buson, SD Alighieri, L Greggio, A Renzini, J Funes, F Bertola

Abstract:

The nature of the UV-bright spike at the center of the otherwise normal galaxy NGC 4552 is investigated by means of both Hubble Space Telescope (HST) imaging (FOC) and spectroscopy (FOS). This central feature-which underwent a recent dramatic UV flare-provides a potential new tool for revealing the presence of massive black holes in normal galaxies. In particular the sub-arcsec FOS spectra of the nucleus suggest that NGC 4552 does harbor an object with mass M > 4 x 10(8) M. within the central 2 pc.
More details

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