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DTSTAMP:20181221T160730Z
LOCATION:D220
DTSTART;TZID=America/Chicago:20181114T103000
DTEND;TZID=America/Chicago:20181114T104500
UID:submissions.supercomputing.org_SC18_sess338_svs105@linklings.com
SUMMARY:Visualizing Outbursts of Massive Stars
DESCRIPTION:Scientific Visualization & Data Analytics Showcase\nVisualizat
 ion, Tech Program Reg Pass\n\nVisualizing Outbursts of Massive Stars\n\nIn
 sley, Jiang, Cantiello, Bildsten, Quataert...\n\nMassive stars play an imp
 ortant role in many astrophysical environments such as star formation and 
 the structure of the interstellar medium in galaxies. However, the structu
 res and mass loss of massive stars, which are crucial to understand the ev
 olution and fate of massive stars, are still mysteries. Global radiation h
 ydrodynamic simulations of an 80 solar mass star envelope were performed o
 n the Argonne Leadership Computing Facility’s supercomputer, Mira, to find
  the answers. In this work, we present visualizations of the data produced
  in these simulations, which show the important role that helium opacity p
 lays in outbursts from massive stars.
URL:https://sc18.supercomputing.org/presentation/?id=svs105&sess=sess338
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