COMMISSION 27 OF THE I. A. U INFORMATION BULLETIN ON VARIABLE STARS NUMBER 246 Konkoly Observatory Budapest 1968 January 10 Veroffentlichungen der Remeis-Sternwarte Bamberg Astronomisches Institut der Universitat Erlangen-Nurnberg Band VII, Nr. 64 A NEW CEPHEID IN THE LMC BV 906 (in the LMC) is detected as variable by H. MEIER (Veroff. Remeis-Sternwarte Bamberg, Bd. VI, Nr. 48, 1967, there position and identification card). First the Harvard plate material (all maxima before JD 2439100, estimated by A. BAUERNFEIND makes possible the derivation of elements: Max=JD 2413847.250+5.^d072575*E Maxima E O-C 2413847.841 0 +0.591 3922.617 15 -0.722 3948.574 20 -0.128 3954.583 21 +0.809 7590.587++ 738 -0.223 7965.607 812 -0.574 2423465.597+ 1896 +0.745 3490.574 1901 +0.359 3667.868 1936 +0.113 3682.875 1939 -0.098 3738.785 1950 +0.014 4408.850 2082 +0.499 4418.800++ 2084 +0.304 4824.683 2164 +0.381 6011.336 2398 +0.051 6245.582 2444 +0.959 6264.557 2448 -0.357 6341.332 2463 +0.330 6412.253+ 2477 +0.235 6427.255 2480 +0.019 6452.220 2485 -0.379 6453.220 2485 +0.621 6594.599+ 2513 -0.032 6635.562+ 2521 +0.350 6960.608 2585 +0.752 7310.577 2654 +0.713 7421.312++ 2676 -0.149 .344++ 2676 -0.117 7422.272 2678 +0.811 7426.296 2677 -0.237 .329 2677 -0.204 .363 2677 -0.170 .396 2677 -0.137 .448 2677 -0.085 .555 2677 +0.022 7457.277 2683 +0.308 .311 2683 +0.362 .349 2683 +0.380 .382 2683 +0.413 .436 2683 +0.467 .469 2683 +0.500 .502 2683 +0.533 .535 2683 +0.566 7670.574 2723 +0.702 7700.556++ 2731 +0.104 7730.521 2737 -0.367 7746.482+ 2740 +0.376 7747.424+ 2740 +1.318 7756.338 2742 +0.085 7776.524 2746 -0.027 7786.315 2748 -0.371 7802.499+ 2751 +0.598 .552+ 2751 +0.648 7807.283+ 2752 +0.307 .317+ 2752 +0.341 .365+ 2752 +0.389 .399+ 2752 +0.423 .443+ 2752 +0.467 .476+ 2752 +0.500 .517+ 2752 +0.541 .549 2752 +0.573 7808.282 2752 +1.306 .317 2752 +1.341 .377 2752 +1.401 .402 2752 +1.426 8035.597 2797 +0.355 8157.460 2821 +0.476 8405.640 2870 +0.100 8776.584 2943 +0.746 8780.585 2944 -0.326 9202.383 3027 +0.448 9217.448++ 3030 +0.296 9222.409++ 3031 +0.184 9223.406 3031 +1.181 9228.404 3032 +1.107 9349.242+ 3056 +0.203 9517.624 3089 +1.190 9526.598++ 3091 +0.019 9577.384+ 3101 +0.079 9587.337+ 3103 -0.113 9674.309 3120 +0.625 9881.575 3161 -0.085 9927.447+ 3170 +0.134 9938.541 3172 +0.919 2430023.355 3189 -0.337 0318.394 3247 +0.493 .554 3247 +0.653 0373.270 3258 -0.429 .325 3258 -0.374 .392 3258 -0.307 0647.582+ 3304 -0.036 0749.276 3332 +0.206 0977.564++ 3377 +0.228 .612++ 3377 +0.276 1109.457+ 3403 +0.234 1297.632 3440 +0.724 1317.599 3444 +0.401 1327.634+ 3446 +0.291 1328.570 3446 +1.227 .617 3446 +1.274 1332.587+ 3447 +0.171 .626+ 3447 +0.210 1657.649 3511 +0.588 1677.644++ 3515 +0.293 1682.637+ 3516 +0.213 1697.559+ 3519 -0.082 1702.562++ 3520 -0.152 1703.629 3520 +0.915 1708.613 3521 +0.826 1712.517 3522 -0.342 1713.545 3522 +0.686 1734.511 3526 +1.362 2012.641 3581 +0.500 2027.647+ 3584 +0.288 2037.641 3586 +0.137 2042.647 3587 +0.071 2053.628 3589 +0.906 2058.600 3590 +0.806 2067.621 3592 -0.318 2129.569 3604 +0.759 2509.307++ 3679 +0.054 2838.602 3744 -0.369 2884.277+ 3753 -0.347 .322+ 3753 -0.302 .365+ 3753 -0.259 .418+ 3753 -0.206 2915.336+ 3759 +0.277 2940.363+ 3764 -0.059 .413+ 3764 -0.009 .457 3764 +0.035 2941.291 3764 +0.869 .343 3764 +0.921 .385 3764 +0.963 .433 3764 +1.011 3153.625+ 3806 +0.155 9139.377+ 4986 +0.268 9150.338 4988 +1.084 9164.273+ 4991 -0.199 9169.281 4992 -0.263 9174.274 4993 -0.343 9175.282 4993 +0.665 9180.280 4994 +0.590 9184.283 4995 -0.479 9195.258+ 4997 +0.351 9200.256++ 4998 +0.276 9205.244+ 4999 +0.192 9210.243++ 5000 +0.118 9215.444 5001 +0.246 9225.256 5003 -0.087 9230.226 5004 -0.189 9236.235 5005 +0.747 9443.562+ 5046 +0.099 Probable a hump near phase 0.25. Light variation approximately 14.^m9-16.^m0 with the minimum about phase 0.75. The brightness is too large or the period is too short for the usual periodluminosity relation. Very good maxima are signified by crosses. Remeis-Observatory Bamberg, 1987 Dez. 31 W. STROHMEIER