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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

Observed trend in the star formation history and the dark matter fraction of galaxies at redshift $z\approx0.8$

(2015)

Authors:

Shravan Shetty, Michele Cappellari

MEASURING THE MASS OF THE CENTRAL BLACK HOLE IN THE BULGELESS GALAXY NGC 4395 FROM GAS DYNAMICAL MODELING

The Astrophysical Journal American Astronomical Society 809:1 (2015) 101

Authors:

Mark den Brok, Anil C Seth, Aaron J Barth, Daniel J Carson, Nadine Neumayer, Michele Cappellari, Victor P Debattista, Luis C Ho, Carol E Hood, Richard M McDermid

THE AGES, METALLICITIES, AND ELEMENT ABUNDANCE RATIOS OF MASSIVE QUENCHED GALAXIES AT * * Based on data collected at the Subaru telescope, which is operated by the National Astronomical Observatory of Japan. (Proposal IDs: S09A-043, S10A-058, and S11A-075.)

The Astrophysical Journal American Astronomical Society 808:2 (2015) 161

Authors:

M Onodera, CM Carollo, A Renzini, M Cappellari, C Mancini, N Arimoto, E Daddi, R Gobat, V Strazzullo, S Tacchella, Y Yamada

Measuring the mass of the central black hole in the bulgeless galaxy NGC 4395 from gas dynamical modeling

(2015)

Authors:

Mark den Brok, Anil C Seth, Aaron J Barth, Daniel J Carson, Nadine Neumayer, Michele Cappellari, Victor P Debattista, Luis C Ho, Carol E Hood, Richard M McDermid

General spherical anisotropic Jeans models of stellar kinematics: including proper motions and radial velocities

(2015)

Abstract:

Cappellari (2008) presented a flexible and efficient method to model the stellar kinematics of anisotropic axisymmetric and spherical stellar systems. The spherical formalism could be used to model the line-of-sight velocity second moments allowing for essentially arbitrary radial variations in the anisotropy and general luminous and total density profiles. Here we generalize the spherical formalism by providing the expressions for all three components of the projected second moments, including the two proper motion components. A reference implementation is now included in the public JAM package available at http://purl.org/cappellari/software.

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