How high energy fluxes may affect Rayleigh–Taylor instability growth in young supernova remnants
C. C. Kuranz, H.-S. Park, C. M. Huntington and 25 more
Nature Communications · 2018
doi:10.1038/s41467-018-03548-7 (opens in a new tab)
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Abstract
Radiation and conduction are generally considered as the main energy transport mechanisms for the evolution of early supernova remnants. Here the authors experimentally show the role of electron heat transfer on the growth of Rayleigh–Taylor instability in young supernova remnants.
Abstract licence: CC BY-NC-ND
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