General relativity predicts that binary systems of stars produce gravitatio
nal waves of significant intensity. Here we are particularly interested in
the cataclysmic variable binaries (CVs). These systems emit low frequency g
ravitational waves, f < 10(-3) Hz. We present here a catalog of CVs and arg
ue that part of them are capable of being detected by the Laser Interferome
ter Space Antenna (LISA).