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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.

Julien Devriendt

Professor of Astrophysics

Research theme

  • Astronomy and astrophysics
  • Particle astrophysics & cosmology

Sub department

  • Astrophysics

Research groups

  • Beecroft Institute for Particle Astrophysics and Cosmology
  • Cosmology
  • Galaxy formation and evolution
julien.devriendt@physics.ox.ac.uk
Telephone: 01865 (2)73307
Denys Wilkinson Building, room 555D
  • About
  • Teaching
  • Publications

Cloud Dispersal in Turbulent Flows

(2006)

Authors:

F Heitsch, AD Slyz, JEG Devriendt, A Burkert
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Wide field spectrograph concepts for the European Extremely Large Telescope

Proceedings of SPIE - The International Society for Optical Engineering 6269 II (2006)

Authors:

G Moretto, R Bacon, JG Cuby, F Hammer, P Amram, S Blais-Ouellette, PE Blanc, J Devriendt, B Epinat, T Fusco, P Jagourel, O Hernandez, JP Kneib, I Montilla, B Neichel, E Pécontal, E Prieto, M Puech

Abstract:

We report on the science case high level specifications for a wide field spectrograph instrument for an Extremely Large Telescope (ELT) and present possible concepts. Preliminary designs are presented which resort to different instrument concepts: monolithic integral field (IFU), multi-IFU, and a smart tunable filter. This work is part of the activities performed in the work package 'Instrumentation' of the 'ELT Design Study', a programme supported by the European Community, Framework Programme 6.
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The birth of molecular clouds:formation of atomic precursors in colliding flows

Astrophysical Journal 648 (2006) 1052-1065

Authors:

AD Slyz, Fabian Heitsch, Julien Devriendt, Lee Hartmann
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Non-Standard Structure Formation Scenarios

Astrophysics and Space Science Kluwer Academic Publishers 284 (2006) 335-340

Authors:

A Knebe, B Little, R Islam, J Devriendt, A Mahmood, J Silk

Abstract:

Observations on galactic scales seem to be in contradiction with recent high resolution N-body simulations. This so-called cold dark matter (CDM) crisis has been addressed in several ways, ranging from a change in fundamental physics by introducing self-interacting cold dark matter particles to a tuning of complex astrophysical processes such as global and/or local feedback. All these efforts attempt to soften density profiles and reduce the abundance of satellites in simulated galaxy halos. In this contribution we are exploring the differences between a Warm Dark Matter model and a CDM model where the power on a certain scale is reduced by introducing a narrow negative feature (''dip''). This dip is placed in a way so as to mimic the loss of power in the WDM model: both models have the same integrated power out to the scale where the power of the Dip model rises to the level of the unperturbed CDM spectrum again. Using N-body simulations we show that that the new Dip model appears to be a viable alternative to WDM while being based on different physics: where WDM requires the introduction of a new particle species the Dip stems from a non-standard inflationary period. If we are looking for an alternative to the currently challenged standard LCDM structure formation scenario, neither the LWDM nor the new Dip model can be ruled out with respect to the analysis presented in this contribution. They both make very similar predictions and the degeneracy between them can only be broken with observations yet to come.
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Modelling the galaxy bimodality: shutdown above a critical halo mass

Monthly Notices of the Royal Astronomical Society 370:4 (2006) 1651-1665

Authors:

JEG Devriendt, Cattaneo, A., Dekel A., Guiderdoni B.
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