Title: Complete evolution of a supernova remnant
Abstract: Understanding the supernovae remnants or shocks in general reveals a great deal about the interstellar medium (ISM) including hints to the galactic evolution. Dynamics and evolution of SN remnants is a classical problem and have been studied numerous times in the literature but never with a self-consistent atomic physics. In this talk, I will discuss our efforts to study the textbook problem but with a self-consistent chemical network that is coupled to hydrodynamics and radiative transfer.
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Meeting ID: 978 019 999
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