COMMISSION 27 OF THE I. A. U.
        INFORMATION BULLETIN ON VARIABLE STARS
                    Number 2382

                                    Konkoly Observatory
                                    Budapest
                                    12 August 1983

                                    HU ISSN 0374-0676





        BV PHOTOMETRY OF THE SUPERNOVA 1982 IN NGC 2268




  BV photometry of the supernova in NGC 2268 discovered by Wild (1982) is
reported.



          Table I
BV photometry of the supernova
------------------------------
Date       UT      B     V
------------------------------
27/2/82   21h17m       14.00
27/2/82   22 50        14.05
01/3/82   19 30        14.05
02/3/82   20 05        14.40
06/3/82   21 02  15.4
06/3/82   20 18        14.45
14/3/82   19 43  16.00
14/3/82   20 15        14.65
15/3/82   20 15  16.05
15/3/82   20 41        14.65
24/3/82   20 15  16.45
24/3/82   21 41        15.30
26/3/82   20 10  16.50
26/3/82   21 56        15.35
14/4/82   20 58  16.85
14/4/82   20 15        15.80
18/4/82   21 08  16.95
14/5/82   21 49        16.1)
-----------------------------

The observations were obtained with the 0.4 m Schmidt telescope in
Metzerlen on plates 103a-O, 103a-D and filters Schott 2 mm GG 13 in B and
Schott 2 mm GG 11 in V.

                          [FIGURE 1]

   Figure 1: B light curve of SN 1982 Typ I in NGC 2268

                          [FIGURE 2]

   Figure 2: SN, NGC 2268 and comparison sequence

                   Table II
                Comparison sequence
----------------------------------------
No.       B      V    No.     B       V
----------------------------------------
  1     15.4   14.5   34    16.0    14.6
  2     15.3   14.0   35    16.1    15.3
  3     14.6   14.0   36    16.0    15.1
  4     15.9   15.0   37    16.1    15.1
  5     16.9   16.1   38    16.0    15.0
  6     17.0   16.4   39    16.0    14.8
  7     15.7   14.7   40    13.7    12.7
  8     15.9   15.2   41    16.8
  9     16.3   15.6   42    17.3
 10     16.9   16.2   43    16.4
 11     17.1   16.1   44    17.0
 12     14.7   13.6   45    16.1
 13     14.9   13.5   46    17.2
 14     16.6   15.5   47    14.8
 15     15.2   14.3   48    16.8
 16     16.2   15.5   49    15.7
 17     16.5   15.1   50    17.2)
 18     16.8   15.8   51    14.7
 19     16.4   15.7   52    14.5
 20     14.6   13.3   53    14.9
 21     16.3   15.5   54    17.4    16.8
 22     16.2   15.3   55    16.4    15.6
 23     16.5   15.5   56    16.5    15.8
 24     17.2   16.3   57    16.1
 25     16.2   15.4   58    17.5)
 26     15.1   14.1   59    17.5    16.9
 27     15.2   14.3   60    16.7    16.0
 28     15.1   14.1   61    17.2    16.4
 29     16.1   15.4   62    16.6    15.8
 30     17.3   16.6   63    16.5    15.6
 31     17.8)  16.5   64    15.2
 32     16.4   15.6   65    13.4
 33     16.3   15.5
-----------------------------------------



The comparison sequence was derived from the North Polar Sequence and two
fields of stars between the Polar and the comparison sequence.




                   R. CADONAU

                  Dr. C. TREFZGER





References:
Barbon, R. et al.: 1982, IAU Circ., No. 3671 [BIBCODE 1982IAUC.3671....1S ]
Wild, P.: 1982, IAU Circ., No. 3667 [BIBCODE 1982IAUC.3667....1W ]
Wood, R.: 1982, IAU Circ., No. 3678 [BIBCODE 1982IAUC.3678....3W ]