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SUMMARY:Galaxy Evolution in 3-D - Professor Lisa Kewley (ANU)
DTSTART:20140213T163000Z
DTEND:20140213T173000Z
UID:TALK50466@talks.cam.ac.uk
CONTACT:Simon Hodgkin
DESCRIPTION:*Abstract*\n\nThroughout the history of the universe\, shocks 
 and large-scale gas flows have moulded the arms of spiral galaxies\, forme
 d the bulges of the most massive galaxies in the universe\, fed supermassi
 ve black holes in the centres of galaxies\, fuelled generation upon genera
 tion of new stars\, and enriched the intergalactic medium with metals.  I 
 will present the latest results from our large local 3D survey to understa
 nd the relationship between galactic-scale outflows\, star-formation\, and
  active galactic nuclei in galaxies as a function of environment and redsh
 ift.  For local galaxies\, we use multi-object integral field spectroscopy
  to build the largest sample of galaxies with wide 3-dimensional imaging s
 pectroscopy.  We probe the early universe by combining gravitational lensi
 ng with new infrared 3-dimensional imaging spectroscopic technology.  Grav
 itational lensing allows us to probe the fundamental processes occurring w
 ithin actively forming galaxies just 4 billion years after the Big Bang.  
 In this lecture\, I will present the latest results of our large survey to
  track how the star formation\, chemical abundances\, and galactic-scale o
 utflows changed within galaxies over the past 11 billion years.\n
LOCATION:Sackler Lecture Theatre\, IoA (tea at 4:00 pm)
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