  In this work we present full sets of solutions for rotating charged boson
stars with different coupling values. By adopting local comoving coordinates,
we are able to find expressions for the effective hydrodynamic quantities of
the fluids as seen by this class of observers. We show that not only is the
energy density non zero at the center, for the uncharged case it has a local
maximum at the core from which it decreases until the point of local minimum
where its variation is discontinuous. For the first time, it is reported how
rotating boson stars, charged and uncharged, are completely anisotropic fluids
featuring three different pressures. Furthermore, the character of the
electromagnetic fields is analyzed.
