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TITLE:
Exploring the asymmetry of core-collapse supernovae
SPEAKER:
Professor John Blondin,
TIME: Thursday Nov. 2, 2006 at 4:00 PM
PLACE: George P. Williams, Jr. Lecture Hall, (Olin 101)
Refreshments will be served at 3:30 PM in the lounge.
All interested persons are cordially invited to attend.
Modern astronomical observations are revealing a
Universe of stellar objects that are dramatically asymmetric
and time-dependent. A particularly energetic example is
a core-collapse supernovae, where the death of a massive star
generates a blastwave of 1044 Joules that propagates out through
the surrounding interstellar medium for several thousand years.
Using large-scale computer simulations, we will examine
several examples where dynamical instability and/or turbulent
processes dramatically alter the evolution of supernovae and
their remnants. Unexpected results from these multidimensional
simulations include the spinning up of pulsars via shocked accretion
flow and the formation of 'jets' in otherwise spherical explosions.
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100 Olin Physical Laboratory, 7507 Reynolda Station
Wake Forest University
Winston-Salem, NC 27109-7507
Phone: (336) 758-5337, FAX: (336) 758-6142
E-mail: wfuphys@wfu.edu
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