COMMISSION 27 OF THE I.A.U. INFORMATION BULLETIN ON VARIABLE STARS Number 3287 Konkoly Observatory Budapest 3 February 1989 HU ISSN 0374 - 0676 PG 0818+513 - AN ECLIPSING BINARY Observations on 15 plates taken with the astrograph 400/1600 of Sonneberg Observatory show that PG 0818+513 is eclipsing with an amplitude of about 1.5 mag. The magnitude estimates are given in Table I. Table I Magnitude estimates of PG 0818+513 J.D. J.D. 2446700+ B 2446700+ B 62.393 14.63m 64.365 14.50m .430 14.55 .456 15.68 .496 14.55 .561 15.02 .564 14.08 73.403 14.25 63.392 14.98 .450 14.38 .462 14.80 .469 14.42 .606 14.94 .603 14.57 99.627 14.38 The magnitudes have been derived using the sequence of Andronov (1986). The light curve (Figure 1) is based on the preliminary elements min = 2446764.460+ 0.577d*E (?) [FIGURE 1] Figure 1 Provisional light curve of PG 0818+513. Dots: J.D. 244 6762...64, crosses: J.D. 244 6773 Because of the sparseness of the data, the length of the orbital period is still uncertain. If the shoulder near phase 0.75 proves to be real, it would suggest that the bright spot is more luminous than the accretion disk, as is the case in objects with small mass accretion rates, that is, in most of the dwarf novae. But eruptions on PG 0818+513 have neither been observed on Moscow (Andronov 1986) nor on Sonneberg plates so far. GEROLD A. RICHTER Sternwarte Sonneberg Zentralinstitut fur Astrophysik der AdW der DDR Reference: Andronov, I.L. 1986, Astron. Tsirk., No. 1418. [BIBCODE 1986ATsir1418....1A ]