Cite
Kuranz CC, Park HS, Huntington CM, et al. How high energy fluxes may affect Rayleigh-Taylor instability growth in young supernova remnants. Nat Commun. 2018;9(1):1564doi: 10.1038/s41467-018-03548-7.
Kuranz, C. C., Park, H. S., Huntington, C. M., Miles, A. R., Remington, B. A., Plewa, T., Trantham, M. R., Robey, H. F., Shvarts, D., Shimony, A., Raman, K., MacLaren, S., Wan, W. C., Doss, F. W., Kline, J., Flippo, K. A., Malamud, G., Handy, T. A., Prisbrey, S., Krauland, C. M., Klein, S. R., Harding, E. C., Wallace, R., Grosskopf, M. J., Marion, D. C., Kalantar, D., Giraldez, E., & Drake, R. P. (2018). How high energy fluxes may affect Rayleigh-Taylor instability growth in young supernova remnants. Nature communications, 9(1), 1564. https://doi.org/10.1038/s41467-018-03548-7
Kuranz, C C, et al. "How high energy fluxes may affect Rayleigh-Taylor instability growth in young supernova remnants." Nature communications vol. 9,1 (2018): 1564. doi: https://doi.org/10.1038/s41467-018-03548-7
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. How high energy fluxes may affect Rayleigh-Taylor instability growth in young supernova remnants. Nat Commun. 2018 Apr 19;9(1):1564. doi: 10.1038/s41467-018-03548-7. PMID: 29674695; PMCID: PMC5908785.
Copy
Download .nbib