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\begin{itemize}  \item Ap/Bp stars statistics \cite{Hubrig_2000} (Fields exist already on the PMS \cite{Wade_2005}, it's unclear if a correlation between magnetic field strength and stellar mass is present, but probably not \cite{Landstreet_2007}. The data is consistent with flux conservation for most (but not all) Ap stars, or with modest decline in flux with age \cite{Landstreet_2008})   \item Thermohaline mixing suppression from B-fields \cite{Charbonnel_2007} \cite{Charbonnel_2007}. Requires B~$10^5$ G around the H-shell. From surface abundance observations it seems to occur in 5-10\% of red giants. Roughly consistent with the Ap stars statistics.  \item Pulsating RoAp stars. BField/pulsation alignments  \item Magnetic WD statistics   \item Predictions for Clump stars