Results 151 to 160 of about 68,500 (261)
, 2010 During the evolution on the AGB, S-type stars are the first objects to experience s-process nucleosynthesis and third dredge-ups, and therefore to exhibit sprocess signatures in their atmospheres. Their significant mass loss rates (10^-7 to 10^-6 M*/year)
Goriely, Stéphane +5 more
core
Xenon-metal pair formation in UO2 investigated using DFT+U [PDF]
arXivA recent experimental study on a spent uranium dioxide (UO2) fuel sample from Belgium Reactor 3 (BR3) identified a unique pair structure formed by the noble metal phase (NMP) and fission gas (xenon [Xe]) precipitate. However, the fundamental mechanism behind this structure remains unclear.
arxiv
A Search for Technetium in the BA II Star ζ Capricorni [PDF]
, 1974 Ann Merchant Boesgaard, Robert A. Fesen
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DETERMINATION OF TOTAL FISSION PRODUCT MOLYBDENUM, TECHNETIUM, AND TELLURIUM IN ICPP WASTE TANKS
, 1960 W.J. Maeck, F.W. Dykes, Shigeo Yamamura
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