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PRODID:UW-Madison-Physics-Events
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SEQUENCE:0
UID:UW-Physics-Event-8492
DTSTART:20231102T203000Z
DTEND:20231102T213000Z
DTSTAMP:20260414T045101Z
LAST-MODIFIED:20231102T130231Z
LOCATION:4421 Sterling Hall
SUMMARY:Electromagnetic Transients in the Disks of Active Galactic Nuc
 lei\, Astronomy Colloquium\, Rosalba Perna\, Stony Brook University
DESCRIPTION:The disks of Active Galactic Nuclei (AGNs) have emerged as
  interesting<br>\nenvironments for the evolution of stars and the comp
 act objects they leave<br>\nbehind. The very high density of the mediu
 m\, combined with  torques from the<br>\ngas\, yield evolutionary path
 s for main sequence stars which<br>\ndiffer from those in typical gala
 xies.<br>\nWell known transient phenomena such as long and short GRBs 
 may have<br>\na different-than-usual appearance when emerging from AGN
  disks\, and<br>\nnew astrophysical phenomena\, such as the accretion 
 induced collapse<br>\nof neutron stars to black holes\, may be commonp
 lace in AGN disks. 
URL:https://www.physics.wisc.edu/events/?id=8492
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