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Optimization of isotope composition of fusion plasmas
2011
Nuclear Fusion
Early observations of supernova light curves are powerful tools for shedding light on the pre-explosion structures of their progenitors and their mass-loss histories just prior to explosion. Some core-collapse supernovae that are detected during the first days after the explosion prominently show two peaks in the optical bands, including the R and I bands, where the first peak appears to be powered by the cooling of shocked surface material and the second peak is clearly powered by radioactive
doi:10.1088/0029-5515/51/6/063013
fatcat:m2rsmzx3z5eothgkfurajomvuy