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SUMMARY:Massive galaxy growth from 3D studies - Natasha Foerster-Schreiber
  (MPI for Extraterrestrial Physics)
DTSTART:20140211T163000Z
DTEND:20140211T173000Z
UID:TALK49804@talks.cam.ac.uk
CONTACT:David Titterington
DESCRIPTION:Spatially- and spectrally-resolved studies have provided new a
 nd unique insights into the physical and dynamical processes that drive th
 e star formation and mass assembly of galaxies since as early as a few bil
 lion years after the Big Bang.  I will present key results from near-IR in
 tegral field spectroscopic studies of redshift x ~ 1 1 – 3 galaxies (wit
 h instruments such as SINFONI and KMOS at the VLT) and highlight synergies
  with observations at other wavelengths (notably with HST\, IRAM and Hersc
 hel).  I will discuss implications on the nature\, star formation and gas 
 properties\, feedback mechanisms\, and life cycle of galaxies at the heyda
 y of massive galaxy formation.\n
LOCATION:Sackler Lecture Theatre\, Institute of Astronomy
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