COMMISSION 27 OF THE I. A. U INFORMATION BULLETIN ON VARIABLE STARS NUMBER 261 Konkoly Observatory Budapest 1968 March 18 Veroffentlichungen der Remeis-Sternwarte Bamberg Astronomisches Institut der Universitat Erlangen-Nurnberg Band VII, Nr. 66 NEW BRIGHT SOUTHERN BV-STARS On sky patrol plates of the Bamberg Southern Station 13 further stars were found whose variability seems to be real as can be seen from the material available now. BV 1050 - BV 1089 : vid. Veroffentlichungen der Remeis-Sternwarte Bamberg, vol. VII, Nr. 59 (These stars are faint, no catalogue stars) A_pg BV 1090=BD -09d1609(8.^m5)=HD 48 419(B_9) 0.^m45 BV 1091=BD -05d1892(9.^m0)=HD 51 569(B_8) 0.^m30 BV 1092=BD -15d1695(8.^m2)=HD 55 538(B_2)=CSV 102550 0.^m35 BV 1093=CoD -31d4663(9.^m3)=CAP -31d1624(8.^m7) 0.^m40 BV 1094=CAP -56d1418(7.^m6)=HD 63 203(A_0) 0.^m30 BV 1095=CoD -44d3871(9.^m3)=HD 65 293(A_0) 0.^m40 BV 1096=CAP -68d0761(9.^m5)=CoD -68d0540(9.^m0)=CSV 1276=S 4898 0.^m30 BV 1097=CoD -37d4833(9.^m6)=CAP -37d2534(9.^m2) 1.^m20 BV 1098=CAP -54d2265(9.^m2)=CoD -54d2793(9.^m7) 0.^m30 BV 1099=CoD -44d6252(7.^m3)=HD 88 303(K_2) 0.^m30 BV 1100=CAP -67d1907(8.^m8)=HD 105 355(B_9) 0.^m30 BV 1101=CAP -54^5772(8.^m8) =HD 120 738(B_9) 0.^m40 BV 1102=CoD -46^9108(10^m) =HD 123 460(A_3) 0.^m30 [FIGURE 1] BV 1095=CoD -44d3871(9.^m3)=HD 65 293(A_0) Min=JD 2434336.450+2.^d398735*E Minima E O-C 2428820.593(S,-) -2299.5 +0.034 8897.548(S,=) -2267.5 +0.230 8904.438(S) -2264.5 -0.076 3434336.465(S) 0 +0.015 4485.353(S,-) 62 +0.181 4533.246(S,-) 82 +0.100 8492.225 1732.5 -0.033 8817.314 1868 +0.027 8823.302 1870.5 +0.018 9118.499(1/2) 1993.5 +0.171 9178.332 2018.5 +0.036 9196.276 2026 -0.011 9202.254 2028.5 -0.030 9563.265 2179 -0.029 Ampl. 0.^m45, secondary minimum as deep as primary minimum, EA BV 1097=CoD -37d4833(9.^m6)=CAP -37d2534(9.^m2) Min=JD 2434302.525+1.^d052565*E Minima E O-C 2434302.590(S,-) 0 +0:065 4311.498(S ) 8.5 +0.026 4418.349(S) 110 +0.042 4422.504(S,+) 114. -0.013 4488.328(S) 176.5 +0.025 8739.551(1/3) 4215.5 -0.062 8786.409(3/4) 4260 -0.043 9525.386 4962 +0.034 9126.364 4963 -0.041 9535.355 4971.5 +0.003 9562.256(3/4) 4997 +0.064 9563.265 4998 +0.020 Ampl. 1.^m2, with very deep secondary minimum, EW or EB BV 1101=CAP -54d5772(8.^m8)=HD 120738(B_9) Min=JD 2428257.475+0.^d5807835*E Minima E O-C 2428257.506(S) 0 +0.031 8275.444(S) 31 -0.035 8661.433(S) 695.5 +0.023 8743.250(S) 836.5 -0.050 8777.248(S) 895 -0.028 2434516.296(S) 10776.5 +0.008 4532.246(S) 10804 -0.014 4537.503(S) 10813 +0.016 4540.384(S) 10818 -0.007 8475.501 17593.5 +0.011 8498.451 17633 +0.021 8528.335 17684.5 -0.006 8551.244 17724 -0.038 .288 17724 +0.006 8590.204++ 17791 +0.010 8879.403 18289 -0.021 8914.300 18349 +0.029 8932.258+ 18380 -0.018 9202.383 18845 +0.043 9204.378 18848.5 +0.005 9210.488 18859 +0.017 9235.410 18902 -0.035 9265.358 18953.5 +0.003 9270.308++ 18962 +0.016 9566.528+ 19472 +0.037 Ampl. 0.^m40, With a very deep (3/4) secondary minimum, EW (S)=Sonneberg (H. GESSNER) Bamberg, Remeis-Observatory February 28, 1968 W. STROHMEIER, H. OTT, E. SCHOFFEL