COMMISSIONS 27 AND 42 OF THE IAU INFORMATION BULLETIN ON VARIABLE STARS Number 3879 Konkoly Observatory Budapest 13 May 1993 HU ISSN 0374 - 0676 A NEW VARIABLE STAR GSC 4383.0384 Observing supernova 1993J in the evening April 16,1993 at 19:15 UT, Kamil Hornoch and Jan Kysely (at 19:12 UT) independently noticed a brightness change of a star plotted in a special AAVSO chart for SN 1993J at NGC 3031 (M81). The star is some 9.7' north and 4.7' west with respect to the center of M81 galaxy. The star's number in the Guide Star Catalog [1] is 4383.0384, alpha = 9h54m28.9s, delta = +69d13'22" (equinox 2000.0) its brightness is given there as 10.80 mag. The star is not included in the General Catalogue of Variable Stars (2) nor in the New Catalogue of Suspected Variable Stars (3). Visual observation by K. Hornoch, J. Kysely and other visual observers will be published in (4). K. Hornoch's message arrived immediately at the N. Copernicus Observatory and Planetarium in Brno, where the star was measured the same night by the photometer (uncooled EMI 6256 photomultiplier) of our 0.4 m telescope and variability of this star was definitely confirmed. In the course of photoelectric measurements HD 86677 (V=7.876 mag, B-V=+0.510, Hipparcos Input Catalogue [5]), was used as the comparison star, check stars were HD 85458, HD 85743 and GSC 4383.0565. Their V and B-V data indicate that the comparison star is constant, whereas the GSC 4383.0384 exhibited apparent light variations, when we measured it. Up to now we measured six nights and we caught two maxima and two minima. The V amplitude the star can be estimated at 0.3 mag and period about dozen hours. More detailed information on the photoelectric measurements of the new variable will be published later. Dalibor HANZL Jan KYSELY N. Copernicus Obs. Cs. Armady and Planetarium 258 01 VLASIM 616 00 BRNO Czech Republic Czech Republic (E-mail: HANZLC@CSBRMU11) Kamil HORNOCH Paseky 392 664 31 Lelekovice p. CESKA Czech Republic References: [1] The Guide Star Catalogue, ver. 1.1, 1992, Space Telescope Science Institute, Baltimore. [2] Kholopov, P.N., Samus, N.N., Frolov, M.S., Goranskij, V.P., Gorynya, N.A., Karitskaya, E. A., Kazarovets, E.V., Kireeva, N.N., Kukarkina, N.P., Medvedeva, G.I., Pastukhova, E.N., Perova, N.B., and Shugarov, S.Yu, 1987, General Catalogue of Variable Stars, Vol. III., Nauka, Moscow. [3] Kukarkin, B.V., Kholopov, P.N., Artiukhina, N.M., Fedorovich, V.P., Frolov, M.S., Goranskij, N.A., Gorynya, N.A., Karitskaya, E.A., Kireeva, N.N., Kukarkina, N.P., Kurochkin, N.E., Medvedeva, G.I., Perova, N.B., Ponomareva, G.A., Samus', N.N. and Shugarov, S. Yu, 1982 New Catalogue of Suspected Variable Stars, Nauka, Moscow [4] Contributions of the Nicholas Copernicus Observatory and Planetarium in Brno No. 31. [5] Turon, C., et al., 1992, Hipparcos Input Catalogue. [BIBCODE 1992hicv.book.....T ]