Galaxies - PowerPoint PPT Presentation

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Galaxies

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Collaborators : G. Cecil, C.G. Mundell. Active Galaxies. Perspectives : ... Collaborators : G. Cecil, C.G. Mundell, A.S. Wilson. M51 - OASIS. Active Galaxies ... – PowerPoint PPT presentation

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Title: Galaxies


1
Active galaxies in Lyon
Pierre Ferruit
(yes the title is different)
  • Work conducted at the CRAL Observatoire de Lyon
  • Emmanuel Pécontal, Eric Emsellem and Pierre
    Ferruit
  • International collaborations
  • Heavily 3D-biased

2
Active galaxies
  • Major scientific projects
  • Energetic balance of the ionized gas of the ENLR
  • Kinematics of the ionized gas
  • Observation and modeling of jet / ambient ISM
    interaction
  • From observations
  • 3D spectroscopy, HST, Chandra, VLA
  • to models
  • hydrodynamics radiation transfer

3
Active Galaxies
  • Energetic balance of the ENLR
  • 3D spectroscopy HST imaging in the visible
  • gt Combine line ratio diagnostics with the
    gaseous kinematics

4
Active Galaxies
  • Energetic balance of the ENLR
  • 3D spectroscopy HST imaging in the visible
  • gt Combine line ratio diagnostics with the
    gaseous kinematics

5
Active Galaxies
  • Energetic balance of the ENLR
  • 3D spectroscopy HST imaging in the visible
  • gt Combine line ratio diagnostics with the
    gaseous kinematics
  • Multi-wavelength observations
  • gt Extensive spectral coverage

6
Active Galaxies
  • Energetic balance of the ENLR
  • 3D spectroscopy HST imaging in the visible
  • gt Combine line ratio diagnostics with the
    gaseous kinematics
  • Multi-wavelength observations
  • gt Extensive spectral coverage

7
Active Galaxies
  • Jet / ISM interactions
  • Going for spatially resolved structures
  • gt 3D (OASIS) and HST (STIS  3D )
    observations

8
Active Galaxies
  • Jet / ISM interactions
  • Going for spatially resolved structures
  • gt 3D (OASIS) and HST (STIS  3D )
    observations

9
Active Galaxies
  • Jet / ISM interactions
  • Going for spatially resolved structures
  • gt 3D (OASIS) and HST (STIS  3D )
    observations
  • Using existing models and developing new ones
  • gt extracting the physics from the
    observations
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