Abstract
We report on an extensive on-line nuclear orientation study of the angular distribution of $\ensuremath{\alpha}$ particles emitted in the favored decay of neutron deficient At and Rn nuclei near the $N\phantom{\rule{0ex}{0ex}}=\phantom{\rule{0ex}{0ex}}126$ shell closure. Surprisingly large anisotropies were observed, showing pronounced changes from one isotope to another. Comparing these data with several theoretical models shows that anisotropic $\ensuremath{\alpha}$ emission in favored decays from near-spherical nuclei can well be explained within the shell model, implying that it is mainly determined by the structure of the decaying nucleus.
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