COMMISSION 27 OF THE I.A.U.
               INFORMATION BULLETIN ON VARIABLE STARS
                            Number 1495

                                                      Konkoly Observatory
                                                      Budapest
                                                      1978 October 24


          PHOTOELECTRIC MINIMA OF DI PEGASI

Following are the results of observations made at the Ankara
University Observatory with a 30 cm Maksutov telescope, an EMI
6256 S photomultiplier tube and standard B, V filters:


Hel.Min.J.D.     m.e.   Min.   Colour     E       O-C

2443725.5179  +-.0009   II       V      5072.5   +.0002
     29.4335        2   I        B      5078          8
     29.4333        2   I        V                    6
     56.4831        4   I        B      5116         14
     56.4832        5   I        V                   15
     80.3277        8   II       V      5149.5        2


   The method of Kwee and van Woerden (1956) was used in the
calculations of the times of minima and the associated mean errors.
The last column was calculated using the following formula (Binnendijk 
AJ 78, 97, 1973)

    Min. I. = J.D. 2440114.8356 + 0.7118151*E.


                       ZEKI TUFEKCIOGLU

                  Ankara University Observatory
                       A.U. Fen Fakultesi
                         Ankara-Turkey