${\mathrm{E}}_{6}$ models contain right-handed neutrinos which, if light, should be emitted during stellar collapse. Their interactions with matter involve the exchange of an extra neutral gauge boson ${Z}^{\ensuremath{'}}$. We use data from SN 1987A to place bounds on the mass of this new gauge boson which in ${\mathrm{E}}_{6}$ models can be parametrized in terms of a mixing angle $\ensuremath{\theta}$. The limits obtained are, in general, much stronger than those from accelerator data and lie, except for a narrow band around $\ensuremath{\theta}=\ensuremath{-}14.48\ifmmode^\circ\else\textdegree\fi{}$, at the several TeV mass scale.
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