COMMISSION 27 OF THE I. A. U. INFORMATION BULLETIN ON VARIABLE STARS Number 2363 Konkoly Observatory Budapest 30 June 1983 HU ISSN 0374-0676 OBSERVATIONS OF AT Cnc IN THE YEARS 1982 AND 1983 The star which is probably of cataclysmic type (Meinunger, 1981) was inspected on 18 blue-sensitive plates (ORWO-ZU 21 + GG13 + BG12) obtained with the Schmidt camera 50/70/172 cm of Sonneberg Observatory covering the time intervals between 1982 April 14 and April 26 and 1983 February 15 and March 13. These observations are listed in Table I. The light curve of the star which shows variations over the whole amplitude between m_B=12.6 and m_B=15.9 is given in Figure 1. [FIGURE 1] Table I ----------------------------------- J.D. 244.... m_B J.D. 244... m_B ----------------------------------- 5074.352 15.83 5384.421 15.80 5077.363 15.67 5384.475 15.93 5080.351 12.66 5397.338 12.59 5082.356 12.79 5397.365 12.59 5086.352 15.39 5402.404 15.39 5381.407 15.53 5403.380 15.80 5381.436 15.53 5403.408 15.74 5383.392 15.93 5406.333 15.25 5383.531 15.80 5407.331 12.79 ----------------------------------- The sequence of comparison stars in B is shown in the finding chart of Figure 2. [FIGURE 2] Table II ----------------------------------- Comp. star m_B Comp. star m_B ----------------------------------- a 12.25 e 14.97 b 12.93 f 15.67 c 13.62 g 16.45 d 14.30 ----------------------------------- The magnitudes of these stars which include those given by Romano, and Perissinotto (Romano, Perissinotto, 1968) were obtained on 2 plates by linking to the UBV sequence of the Praesepe cluster and are given in Table II. W. GOTZ Akademie der Wissenschaften der DDR, Zentralinstitut fur Astrophysik, Sternwarte Sonneberg References: Meinunger, L., 1981, Mitt. Verand. Sterne Sonneberg 9, p. 59 [BIBCODE 1981MitVS...9...59M ] Romano, G., Perissinotto, M., 1968, Padova Publ. 151, p. 9