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Persistence of collective behavior at high spin in the N = 88 nucleus 153Tb
Persistence of collective behavior at high spin in the N = 88 nucleus 153Tb
Reaction Rate For Carbon Burning In Massive Stars
Reaction Rate For Carbon Burning In Massive Stars
gamma-soft Ba-146 and the role of nonaxial shapes at N approximate to 90
gamma-soft Ba-146 and the role of nonaxial shapes at N approximate to 90