COMMISSION 27 OF THE I. A. U.
       INFORMATION BULLETIN ON VARIABLE STARS
                   Number 1865

                                  Konkoly Observatory
                                  Budapest
                                  1980 November 12

                                  HU ISSN 0374-0676




   NEW VARIABLE STARS IN THE FIELD OF 9 URSAE MAJORIS



  A survey for the search of new variable stars at high
galactic latitude have been made on the plates taken with
the Schmidt telescope (67/90/210 cm) of Asiago in the field 
around 9i UMa.

  Six new variables have been discovered on ten pairs of
plates examined with the blink. The position (1950) and
the characteristics of these stars are listed in Table I.


                 Table I
   var.     R.A.    1950   D      max.    min. type
GR 300   8h49m00s       +50d15'  15.3    16.8   RR :
GR 301   8 50 13        +49 29.7 14.3    15.8   RR
GR 302   8 55 25        +49 04.2 14.0    15.2   ?
GR 303   8 56 30        +49 30.3 14.4    15.0   RR
GR 304   8 58 40        +49 58.6 13.2    14.4   E :
GR 305   9 03 32        +48 28.5 17.7    18.6   L

                       [FIGURE 1]


  The B magnitudes of the comparison stars have been determined 
by SA 45.It is not possible to derive on the basis
of our material the elements of these stars. Fig 1 shows
the finding charts;north is on the top; 15' of side.



                          GIULIANO ROMANO
                       Istituto di Astronomia
                       dell'Universita di Padova