  We study the rotation curves of ultralight BEC dark matter halos. These halos
are long lived solutions of initially rotating BEC fluctuations. In order to
study the implications of the rotation characterizing these long-lived
configurations we consider the particular case of a boson mass
$m=10^{-23}\mathrm{eV/c}^2$ and no self-interaction. We find that these halos
successfully fit samples of rotation curves (RCs) of LSB galaxies.
