BEGIN:VCALENDAR
VERSION:2.0
CALSCALE:GREGORIAN
PRODID:UW-Madison-Physics-Events
BEGIN:VEVENT
SEQUENCE:0
UID:UW-Physics-Event-8386
DTSTART:20230822T230000Z
DURATION:PT1H0M0S
DTSTAMP:20260414T033339Z
LAST-MODIFIED:20230817T132702Z
LOCATION:Please note the unusual time...Join Zoom Meeting https://berk
 eley.zoom.us/j/91230714547  Meeting ID: 912 3071 4547
SUMMARY:The imprint of their explosions: Using supernova remnants to u
 nderstand stellar death \, Network in Neutrinos\, Nuclear Astrophysics
 \, and Symmetries (N3AS) Seminar\, Katie Auchettl \, University of Mel
 bourne\, Australia
DESCRIPTION:One of the most uncertain aspects related to our understan
 ding of the end points of stellar evolution is the link between the pr
 ogenitor star and the nature of the supernova explosion that the proge
 nitor will undergo. Even though hundreds of supernovae are discovered 
 each year by optical surveys\, these sources are usually too distant t
 o resolve the ejecta and immediate surrounding of the exploded star. H
 owever\, due to their long lifetimes and close proximity\, supernova r
 emnants which are the long lived structures that result from the super
 nova explosion of either a white dwarf or a massive star\, provide us 
 with a unique opportunity to study supernova explosion and dynamics up
  close and in detail. In this talk\, I will highlight some recent adva
 nces that have been made in the understanding of supernovae and their 
 progenitors using multi-wavelength studies of supernova remnants.
URL:https://www.physics.wisc.edu/events/?id=8386
END:VEVENT
END:VCALENDAR