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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 quest for the dominant stellar population in the giant elliptical NGC 5018

ASTR SOC P 230 (2001) 435-436

Authors:

LM Buson, F Bertola, M Cappellari, D Burstein
More details

The Cuspy LINER Nucleus of the S0/a Galaxy NGC 2681

(2000)

Authors:

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

The Quest for the Dominant Stellar Population in the Giant Elliptical NGC 5018

(2000)

Authors:

Lucio M Buson, Francesco Bertola, David Burstein, Michele Cappellari
More details from the publisher

NGC 4672: a new case of an early-type disk galaxy with an orthogonally decoupled core

(2000)

Authors:

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

Ultraviolet imaging of the galaxy cluster CL 0939+4713 (Abell 851) at z = 0.41

Astrophysical Journal 531:2 PART 1 (2000) 684-692

Authors:

LM Buson, F Bertola, M Cappellari, C Chiosi, A Dressler, A Oemler

Abstract:

The first UV F300W and F218W WFPC2 observations of the rich galaxy cluster CL 0939 + 4713 at z = 0.41 are presented and discussed. UV/optical two-color and color-magnitude diagrams of the sources detected in the F300W waveband are constructed. Thanks to preexisting Hubble Space Telescope (HST) optical images of the same field, a morphological classification for the majority of these objects is also provided. Moreover, taking advantage of recent redshift surveys along the CL 0939 + 4713 line of sight, separate diagrams comparing the properties of galaxies belonging to the cluster and to its close projected field are presented. Possible evolutionary effects in the UV from z ∼ 0.4 to the present time are investigated by comparing the rest-frame (mid-UV/optical) colors of galaxies in CL 0939 + 4713 with balloon-borne data of the Coma Cluster, as well as by resorting to suitable galaxy evolution models. Finally, current attempts to constrain the epoch of the UV-upturn onset in evolved populations by means of HST UV observations are discussed.
More details from the publisher

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