COMMISSION 27 OF THE I. A. U.
        INFORMATION BULLETIN ON VARIABLE STARS
                     NUMBER 588

                              Konkoly Observatory
                              Budapest
                              1971 October 20



           HD 184077: ANOTHER RED VARIABLE


      During the course of photoelectric photometry of
AQ Sgr, it was discovered that HD 184077 (RA1970=19h31m40s,
D=1970-16d41'), used as comparison star, was variable. The
light- and colour-curves have been constructed, using
HD 184201 (RA1970=19h31m40s, D1970=+4d58') as comparison
star, of which preliminary magnitude and colours are V=6.32m,
B-V=1.91m, U-B=2.03m. The range of the light variation is
0.30m (s. Figure).


-----------------------------------------------------------------
 JD                               JD
               DeltaV Delta(B-V)                DeltaV Delta(B-V)
2441...                           2441...
-----------------------------------------------------------------
115.502        1.208  -0.248      172.327        1.013    -0.228
118.464        1.216  -0.231      178.392        1.083    -0.246
122.523        1.192  -0.239      180.303        1.071    -0.235
127.440        1.110  -0.222      181.297        1.090    -0.248
131.466        1.042  -0.211      183.294        1.090    -0.248
136.442        0.993  -0.198      185.292        1.145    -0.246
143.419        1.043  -0.222      192.311        1.093    -0.246
146.453        1.054  -0.213      193.298        1.095    -0.246
148.455        1.022  -0.220      194.348        1.068    -0.252
150.457        1.024  -0.215      195.250        1.096    -0.257
151.366        1.005  -0.218      209.316        1.084    -0.237
154.416        0.954  -0.211      210.256        1.075    -0.220
156.418        0.920  -0.196      211.261        1.053    -0.226
161.335        0.929  -0.231      216.308        1.023    -0.224
167.337        1.021  -0.226      217.243        1.003    -0.204
169.324        1.028  -0.228      222.248        1.058    -0.226
----------------------------------------------------------------



                             M. WISSE
                        Republic Observatory
                          Johannesburg


                     [FIGURE 1]