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SUMMARY:The Evolution and Limitations of AGN Feedback in Massive Galaxies 
 - Michael McDonald (MIT)
DTSTART:20210312T113000Z
DTEND:20210312T123000Z
UID:TALK157165@talks.cam.ac.uk
CONTACT:Martin Haehnelt
DESCRIPTION:Energetic feedback from supermassive black holes is thought to
  be responsible for preventing star formation in massive galaxies\, includ
 ing our own Milky Way. The most massive galaxies in the Universe\, which l
 ive at the centers of galaxy clusters\, provide a unique\, "high-contrast"
  opportunity to study the details of this feedback. I will present a summa
 ry of work from our group studying the limitations and details of black ho
 le feedback in massive galaxies\, the evolution of the cooling/feedback ba
 lance over ~10 Gyr\, and what we have learned about lower-mass galaxies by
  studying these most-massive systems. I will finish with a summary of othe
 r cluster research\, and a look ahead to the future of research in this fi
 eld.
LOCATION:via zoom 
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