How high energy fluxes may affect Rayleigh-Taylor instability growth in young supernova remnants.
Kuranz CC, Park HS, Huntington CM, Miles AR, Remington BA, Plewa T, Trantham MR, Robey HF, Shvarts D, Shimony A, Raman K, MacLaren S, Wan WC, Doss FW, Kline J, Flippo KA, Malamud G, Handy TA, Prisbrey S, Krauland CM, Klein SR, Harding EC, Wallace R, Grosskopf MJ, Marion DC, Kalantar D, Giraldez E, Drake RP.
Kuranz CC, et al. Among authors: doss fw.
Nat Commun. 2018 Apr 19;9(1):1564. doi: 10.1038/s41467-018-03548-7.
Nat Commun. 2018.
PMID: 29674695
Free PMC article.