COMMISSION 27 OF THE I. A. U.
    INFORMATION BULLETIN ON VARIABLE STARS
                NUMBER 191

                             Konkoly Observatory
                             Budapest
                             28 March 1967

VEROFFENTLICHUNGEN DER REMEIS-STERNWARTE BAMBERG
     ASTRONOMISCHES INSTITUT DER UNIVERSITAT
             ERLANGEN-NURNBERG
               Band VI, Nr. 44

     ELEMENTS FOR THREE BAMBERG VARIABLES

BV 741 = CAP -53d6010(9.4m) = HD 127 329 (A0)

         Min = JD 242 8328.300 + 2.267 310d . E

        Minima        E        O - C

2428328.290(S)        0       -0.010
   8743.250(S)      183       +0.032
   8752.251(S)      187       -0.036
2434361.574(S)     2661       -0.038
   8234.218(1/2)   4369       +0.046
   8474.508        4475       -0.004
       .553(1/2)   4475       +0.041
   8499.443        4486       -0.010
       .488(1/2)   4486       +0.035
   8524.288(1/3)   4497       -0.105
       .433(1/2)   4497       +0.040
   8549.286(3/4)   4508       -0.047
       .331        4508       -0.002
   8556.285(1/4)   4511       +0.150
   8583.201(1/3)   4523       -0.142
       .246(1/2)   4523       -0.097
   8590.204(1/2)   4526       +0.059
   8880.423(1/2)   4654       +0.062
   8914.300(3/4)   4669       -0.070
       .346        4669       -0.024
   8939.258(3/4)   4680       -0.053
   8964.219        4691       -0.032
   9270.308(3/4)   4826       -0.030
       .353        4826       +0.015

   Ampl. 0.45m, no secondary minimum, EA



BV 799 = CAP -76d329(8.8m) = HD 37 513 (F8)
         Min = JD 242 8778.650 + 2.090 550d .  E

Minima           E            O - C

2428778.618(S)      0        -0.032
2434335.383(S)   2658        +0,051
   8355.438      4581        -0.022
   8380.494(1/2) 4593        -0.052
   8443.266      4623        +0.003
       .410(1/4) 4623        +0.147
   8767.288      4778        -0.010
       .333      4778        +0.035
   8813.271      4800        -0.019
   9118.455(3/4) 4946        -0.055
   9139.334(1/2) 4956        -0.082
       .378      4956        -0.038
   9442.453(1/4) 5101        -0.103
       .497(1/2) 5101        -0.049
       .542      5101        -0.004

   Ampl. 0.35m, no secondary minimum, EA


BV 568 = CAP -65d2960(9.6m)
         Min = JD 243 4365.525 + 1.911 485d . E

Minima             E           O - C
2434365.577(S)     0          +0.052
   4513.608(S)   77.5         -0.057
   4538.379(S)   90.5         -0.135
       .511(S)   90.5         -0.003
   8234.218(1/4) 2024         -0.153
       .265(1/2) 2024         -0.106
   8557.285      2036         -0.023
       .330      2036         +0.022
       .374      2036         +0.066
   8581.245(1/2) 2048.5       +0.043
       .294(1/2) 2048.5       +0.092
   8582.201      2049         +0,043
       .245(3/4) 2049         +0.097
       .290(1/4) 2049         +0.132
   8583.246(1/2) 2049.5       +0.132
       .292(1/4) 2049.5       +0.178
   8605.254      2218         +0.055
   8606.225(1/2) 2218.5       +0.071
   8607.208(3/4) 2219         +0.098


Minima             E             O - C
2438855.460(1/2)   2349         -0.143
       .507(1/2)   2349         -0.096
       .555(3/4)   2349         -0.048
   8878.405(1/2)   2361         -0.136
   8879.403(3/4)   2361.5       -0.094
       .449(3/4)   2361.5       -0.048
   8880.423(3/4)   2362         -0.029
       .474(1/2)   2362         +0.022
   8902.347(1/2)   2373.5       -0.088
   8904.332        2374,5       -0.014
       .376        2374.5       +0.030
   8905.310(3/4)   2375         +0.008
       .358(3/4)   2375         +0.056
       .404(1/2)   2375         +0.102
   8906.355(1/2)   2375.5       +0.097
   8930.254(1/2)   2388         +0.103
       .300(1/2)   2388         +0.149
   9270.353(1/2)   2566         -0.043
       .398(3/4)   2566         +0.002

   Ampl. 0.75m, with a secondary minimum nearly as deep as
the primary minimum, EB

(S) = Sonneberg. Again many thanks to Miss H. GESSNER
                 for her search of minima on Sonneberg
                 Sky Patrol Plates.




Remeis Observatory
Bamberg, March 21, 1967


                         W. STROHMEIER