  We investigate the properties of relativistic stars made of dark energy. We
model stellar structure assuming i) isotropic perfect fluid and ii) a dark
energy inspired equation of state, the generalized equation of state of
Chaplygin gas, as we will be calling it. The mass-to-radius profiles, the tidal
Love numbers as well as the ten lowest radial oscillation modes are computed.
Causality, stability and energy conditions are also discussed.
