COMMISSION 27 OF THE I. A. U. INFORMATION BULLETIN ON VARIABLE STARS Number 1611 Konkoly Observatory Budapest 1979 May 28 DISCOVERY OF A PERIOD IN THE SYMBIOTIC STAR AG DRACONIS AG Dra is a well-known symbiotic star. Its photographic light-curve resembles that of the nova-like stars (Robinson, 1969; Splittgerber, 1974). Since 1955 this star has been in a quiet phase and has shown only small variations about the minimum light. Since February 1974 I have observed AG Dra photoelectrically in U, B, V with the 60cm-reflektor II of Sonneberg Observatory. During this time the star has been slowly variable with small amplitude in V and B, but with large amplitude in U (see Fig.1). The same behaviour was observed by Beljakina (1969) in 1965 ....1967. Beljakina (l.c.) concluded from her observations that the variations were irregular, which, however, is not the case. The U variations are clearly periodic with the following elements: U_max = J.D. 243 8900 + 554d*E. There are good reasons for assuming that all symbiotic stars are binaries containing an evolved red giant and a hot main sequence or white dwarf companion (Bath, 1977; Allen, 1978). But so far only three stars of this class could definitively been shown to be binaries (by T CrB; AR Pav; AG Peg; see Allen 1978), I think that the observations of AG Dra given in this paper could well be explained by binary motion of a hot source. But before a reliable model can be constructed, there are more photoelectric and spectroscopic observations necessary. L. MEINUNGER Sonneberg Observatory of Central Institute for Astrophysik of Academy of Sciences of the DDR References: Allen, D.A. 1978, Anglo-Australian Obs. No. 12 Bath, G.T. 1977, MN 178, 203 [BIBCODE 1977MNRAS.178..203B ] Beljakina, T.S. 1969, Iswest.Krim Obs. 40, 39 Robinson, L. 1969, VS 16, 507 [BIBCODE 1969PZ.....16..507R ] Splittgerber, E., 1974, Mitt. veranderl.Sterne 6, 193 [BIBCODE 1975MitVS...6..193S ] [FIGURE 1]