COMMISSION 27 OF THE I.A.U. INFORMATION BULLETIN ON VARIABLE STARS Number 3209 Konkoly Observatory Budapest 27 June 1988 HU ISSN 0374 - 0676 EF PEGASI Tsesevich et al, (1979) gave a report on this U Geminorum type object, which is separated by only 5" from a 15.5 magnitude star. In order to search for further brightenings, I performed magnitude estimates on about 900 sky patrol plates covering the time interval 1928-1986. Because of the low limiting magnitude of the plates, only the brightness maxima, which are given in Table I could be observed (about 11.6m...12.0m, near the brightness of the comparison star "c" in the paper of Tsesevich et al.). The maximum at J.D. 243 6071 given there was published by Tsesevich et al. (1979). As the maxima recur at rather regular intervals, they can be described with the following elements: Max = 2426335 + 162.5d E. A similar cycle length was conjectured by Hoffmeister (1935). Table I J.D. E O-C 2426333 0 - 2d 6987.88 4 + 2 2430547 26 -13 5781 58 +21 6071 60 -14 7906-11 71 +36 8680 76 - 5 9672 82 +12 2445165 116 -20 The separation of EF Peg from the 5" comparison is, of course, not possible on our plates. Inspecting the figure on page 5 of the paper by Tsesevich et al, (1979), one may suppose that EF Peg belongs to the SU UMa subclass of dwarf novae. This question, however, could not be answered because brightness rises and declines could not be followed up on Sonneberg plates. H. GESSNER Akademie der Wissenschaften der DDR Zentralinstitut fur Astrophysik Sternwarte Sonneberg References: Hoffmeister, C., 1935, Astron. Nachr. 255, 407. [BIBCODE 1935AN....255..401H ] Tsesevich, V.P., Goranskij, V.P., Samus, N.N., Shugarov, S.Yu., 1979, Astron. Tsirk, No. 1043. [BIBCODE 1979ATsir1043....3T ]