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Spectroscopy of the Candidate Pre-CV LTT 560
Authors:Claus Tappert  Boris T Gänsicke  Ronald E Mennickent  Linda Schmidtobreick
Institution:(1) Departamento de Astronomía y Astrofísica, Pontificia Universidad Católica, Casilla 306, Santiago 22, Chile;(2) Department of Physics, University of Warwick, Coventry, CV4 7AL, UK;(3) Departamento de Física, Universidad de Concepción, Casilla 306-C, Concepción, Chile;(4) European Southern Observatory, Casilla, 19001, Santiago 19, Chile
Abstract: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.
Keywords:Spectroscopy  Cataclysmic variables  Evolution
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