Abstract
AbstractDuring a supernova explosion, fluid instabilities are generated because the star is in a hydrodynamically unstable situation, which is like the effects of stirring a fire or blowing air into a hot grill. The resulting mixing of the supernova ejecta may be observable. Here, we briefly discuss the multidimensional simulations of supernovae from very massive stars.
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Schedule a callMore From: Proceedings of the International Astronomical Union. International Astronomical Union
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