Gravitational waves from accreting neutron stars
  We show that accreting neutron stars in binary systems or in Landau-Thorne-Zytkow objects are good candidates for continuous gravitational wave emission. Their gravitational radiation is strong enough to be detected by the next generation of detectors having a typical noise of 10^{-23} Hz^{-1/2}. 
S. Bonazzola, E. Gourgoulhon (DARC, CNRS, Observatoire de Paris)