Nous avons étudié les sections efficaces des réactions (p, xn) pour la formation des isotopes du mercure, de masse comprise entre 197 et 188, séparés par déviation magnétique. Nous avons identifié, mesuré les périodes et l'énergie des principales raies γ des 190Hg, 189Hg, 188Hg et de leurs descendants
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