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SUMMARY:Evolution of the Stellar Initial Mass Function over the Past 10 Gy
 r - Vadim Rusakov
DTSTART:20231018T124000Z
DTEND:20231018T130500Z
UID:TALK207469@talks.cam.ac.uk
CONTACT:Hannah Uebler
DESCRIPTION:This work derives physical properties for ∼10^5 most well-me
 asured galaxies from 1 deg^2 in the COSMOS field. Their spectral energy di
 stributions are modelled assuming a stellar initial mass function (IMF) th
 at depends on the temperature of the gas in star-forming regions. It is fo
 und that galaxies exhibit a continuum of IMF shapes\, most of which are bo
 ttom-lighter than measured in the Milky Way. The change is strongest in st
 ar-bursting galaxies and towards high redshift. Furthermore\, correlations
  of the IMF shape with physical properties and morphologies provide an evo
 lutionary interpretation with hints of distinct modes of star formation in
  galaxies.
LOCATION:The Hoyle Lecture Theatre + Zoom 
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