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We present the results of spectroscopic-- and orbit--sampled photometricobservations of the faint UV-excess object PG 2200+085. The optical CCDphotometry observations of this object were performed by the Russian-Turkish1.5-meter telescope RTT150 at the TUBITAK National Observatory (Turkey). Thelong-slit optical spectroscopy observations with 2.6 A resolution were carriedout by 6-meter telescope BTA at the Special Astrophysical Observatory (Russia).The photometric variations over two nights are almost sinusoidal with anamplitude \Delta m_V = 0.04 m and a period of P = 0.3186 d. Such a light curveis typical of a detached close binary with an illumination effect or theellipsoidal deformation of a secondary star. The observed spectrum clearlydisplays a featureless blue continuum of a hot component and a richabsorption--line and molecular band K--star spectrum. The CaII line profileswith strong emission cores are remarkably similar to those of V471 Tau. Wetentatively classify PG 2200+085 as a pre-cataclysmic binary of the V471 Tautype.Comment: 8 pages, 5 figures, accepted for publication in A&

The new pre-cataclysmic binary PG 2200+085