COMMISSION 27 OF THE I. A. U.
        INFORMATION BULLETIN ON VARIABLE STARS
                     NUMBER 324


                                 Konkoly Observatory
                                 Budapest
                                 1969 January 13


    PHOTOELECTRIC OBSERVATIONS OF NOVA VULPECULAE

      The photoelectric observations of Nova Vulpeculae,
discovered by Alcock on April 15, 1968, have been carried
out from April 25 through September 21 at the 330-mm
reflector in a system close to UBV. The filters used were:
UG2, BG12+GG13 and GG11. The observations were reduced to
the standard UBV system.

              The Data of Observations
JD                V    B-V        U-B    n
2439972.463      5.34 +0.56      -0.36   5
     73.432      5.33 +0.61      -0.39   4
     74.440      5.54 +0.59      -0.42   5
     75.410      5.64 +0.56      -0.41   4
     76.404      5.64 +0.59      -0.42   4
     78.425      5.71 +0.56      -0.45   5
     79.406      5.57 +0.61      -0.43   2
2440002.353      7.28 +0.47      -0.42   4
     03.379      7.35 +0.49      -0.47   3
     32.438      8.25 +0.55      -0.42   2
     33.400      8.13 +0.59      -0.23   3
     34.410      8.24 +0.57      -0.34   3
     56.370      8.63 +0.61      -0.10   3
     59.401      8.75 +0.54      -0.04   3
     60.420      8.76 +0.62      -0.07   3
     87.355      9.14 +0.70      +0.11   3
2440088.377      9.13 +0.79      +0.10   2
     89.402      9.13 +0.77      +0.22   3
     94.387      9.13 +0.81      +0.10   3
     97.400      9.18 +0.84      +0.22   2
    119.327      9.49 +1.02      +0.31   3
    120.290      9.40 +1.04       -      3
    121.246      9.42 +0.96       -      3

n is the number of observations used in the formation of a
mean point for a night.
HD186440 (B9) was used as comparison star with V = 6.04,
B-V = -0.04m, U-B = +0.05.

                              O.P. ABULADZE
November 15, 1968     Abastumani Astrophysical Observatory
                              Mt. Kanobili, USSR