We present preliminary results on spectroscopic data of the candidate pre-cataclysmic variable LTT 560 .
A fit to the flux-calibrated spectrum reveals the temperature of the white-dwarf primary to be T _ { eff } = 7000 - 7500 K , and confirms the result of previous studies on the detection of an M5V secondary star .
The analysis of radial velocity data from spectral features attributed to the primary and the secondary star show evidence for low-level accretion .