It was recently shown by Whinnett & Torres \cite{WT} that the phenomenon of
spontaneous scalarization (SC) in compact objects (polytropes) was accompanied
also by a {\it spontaneous violation of the weak energy condition} (WEC).
Notably, by the encounter of negative-energy densities at several star places
as measured by a static observer. Here we argue that the negativeness of such
densities is not generic of scalar tensor theories of gravity (STT). We support
this conclusion by numerical results within a class of STT and by using three
realistic models of dense matter. However, we show that the angular parts'' of the additional conditions for the WEC to hold $\rho_{\rm eff} + T^{i ({\rm eff})}_{i} \geq 0$ tend to be slightly violated’’ at the outskirts of the
star.

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