COMMISSION 27 OF THE I. A. U. INFORMATION BULLETIN ON VARIABLE STARS Number 2733 Konkoly Observatory Budapest 27 May 1985 HU ISSN 0374 - 0676 BEHAVIOUR OF KR AURIGAE IN THE SEASON 1984/85 The star was measured on 28 blue-sensitive plates (ORWO-ZU21+GG13+BG12) from 20 nights obtained with the 50/70/172 cm Schmidt camera of Sonneberg Observatory, covering the time interval between 2 September 1984 and 12 March 1985, using the comparison star sequence given by Popova (1965). The observations are given in Table I. Table I J.D. mB J.D. mB 244.... 244.... 5946.572 13.10mag 6036.542 13.34mag 6002.529 13.22 6059.471 13.22 6003.542 13.42: 6059.490 13.20 6003.567 13.43 6083.422 13.16 6004.478 13.34 6084.325 13.37: 6004.497 13.32 6084.535 13.26 6005.585 13.12 6093.479 13.22 6005.608 13.14 6104.276 13.36 6006.546 13.42 6108.318 13.12 6006.570 13.27 6109.306 13.20 6031.656 13.38 6110.301 13.15 6034.418 13.32 6113.304 13.30 6034.437 13.50 6116.298 13.68 6036.524 13.52 6137.303 14.08 It can be seen from Figure 1 that most of the time KR Aur is in its maximum light between mB= 13.1m and mB = 13.5m ; and slow temporal light fluctuations are superimposed. At the end of the series a decrease in the brightness from mB= 13.3mag to mB = 14.08mag is indicated. [FIGURE 1] W. GOTZ Akademie der Wissenschaften der DDR, Zentralinstitut fur Astrophysik, Sternwarte Sonneberg DDR Reference: Popova, M., 1965, Peremennye Zvezdy, 15, 534. [BIBCODE 1965PZ.....15..534P ]