How high energy fluxes may affect Rayleigh–Taylor instability growth in young supernova remnants

How high energy fluxes may affect Rayleigh–Taylor instability growth in young supernova remnants

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.

Enregistré dans:
Détails bibliographiques
Auteurs principaux: C. C. Kuranz, H.-S. Park, C. M. Huntington, A. R. Miles, B. A. Remington, T. Plewa, M. R. Trantham, H. F. Robey, D. Shvarts, A. Shimony, K. Raman, S. MacLaren, W. C. Wan, F. W. Doss, J. Kline, K. A. Flippo, G. Malamud, T. A. Handy, S. Prisbrey, C. M. Krauland, S. R. Klein, E. C. Harding, R. Wallace, M. J. Grosskopf, D. C. Marion, D. Kalantar, E. Giraldez, R. P. Drake
Format: article
Langue:EN
Publié: Nature Portfolio 2018
Sujets:
Science
Q
Accès en ligne:https://doaj.org/article/f153b9b02a5a45d6934610dc34ba9b57
Tags: Ajouter un tag
Pas de tags, Soyez le premier à ajouter un tag!

Internet

https://doaj.org/article/f153b9b02a5a45d6934610dc34ba9b57

Documents similaires