COMMISSION 27 OF THE I. A. U. INFORMATION BULLETIN ON VARIABLE STARS Number 2172 Konkoly Observatory Budapest 1982 June 28 HU ISSN 0374-0676 SOME REMARKS ON THE T TAURI STAR DR Tau In supplementing and completing the known light curves (Gotz, 1980) the star was inspected on 26 blue-sensitive and on 33 photovisual sky patrol plates of Sonneberg Observatory covering the time interval between 1980 January 12 and 1982 February 21. The used sequence of comparison stars in B is given in the finding chart in Figure 1. The apparent magnitudes m_B of these stars obtained by linking to the UBV-sequence of the open cluster NGC 1647 (Hoag et al., 1961) are listed in Table I. The comparison stars g,h,i and k are identical with the stars a,b,c and d given by Kholopov (1951). [FIGURE 1] Table I Comp. star m_B Comp. star m_B a 10.95 f 13.30 b 11.37 g 13.72 c 11.87 h 14.20 d 12.33 i 14.65 e 12.83 k 15.08 The extended light curve of DR Tau in B is shown in Figure 2. [FIGURE 2] The star has retained its mean Brightness obviously. But it is remarkable that the strong light depressions which were starting from the bright normal light and which were still observed in the season 1979/80 did probable not appear in the seasons 1980/81 and 1981/82. The crosses drawn in Figure 2 represent magnitudes estimated on 6 objective prism plates obtained with the 50/70/172 cm Schmidt camera of Sonneberg Observatory. More details about the behaviour of DR Tau in the past years will be published in MVS. W. GOTZ Akademie der Wissenschaften der DDR Zentralinstitut fur Astrophysik, Sternwarte Sonneberg References: Gotz, W., 1980, MVS 8, 143 Hoag, A.A., Johnson, H.L., Iriarte, B., Mitchell, R.I., Hallam, K.L., Sharpless, S., 1961, Publ. US Naval Obs., 2nd Ser, Vol. 17., No. VII [BIBCODE 1961PUSNO..17....1H ] Kholopov, P.N., 1951, VS 8, 83