COMMISSIONS 27 AND 42 OF THE IAU INFORMATION BULLETIN ON VARIABLE STARS Number 3776 Konkoly Observatory Budapest 28 September 1992 HU ISSN 0374 - 0676 THE SPECTROSCOPIC BINARITY OF MW CYGNI CONFIRMED The Cepheid variable MW Cyg (P=5.954586d) was found by Szabados (1991) to be a new spectroscopic binary Cepheid candidate on the base of a considerable difference of gamma-velocities among the observations published by Joy (1937), Struve (1945) and Barnes et al. (1988). Since July 1991 we have observed the star with the photoelectric velocity meter (CORAVEL type; Tokovinin 1987). Our first 13 radial velocities for MW Cyg (obtained with the 1-m and 0.6-m telescopes in Simeiz and at Mt. Maidanak) have been included in the catalog of Cepheid radial velocities (Gorynya et al., 1992). We have compared these velocities with those analysed by Szabados and found reasonable agreement with the measurements by Barnes et al. (1988); the older radial velocities showed great scatter and seemed to us to be insufficient to judge on the star's binarity with certainty. This summer we gathered 21 new radial velocity measurements of MW Cyg with the same equipment at he 1-m telescope of the Simeiz International Observatory (Crimea, the Ukraine). The Table contains the velocities measured in 1991-1992 with their internal r.m.s. error estimates. The Figure shows the radial velocity curve (dots-1991, crosses-1992) which definitely confirms the star's spectroscopic binarity. We have been able to mention the fact of the binarity confirmation in a note added in proof to our catalog (Gorynya et al., 1992) [FIGURE 1] Figure 1. Radial velocity curve of MW Cyg from our observations. Dots-1991, crosses-1992. Table 1 Radial velocities of MW Cygni HJD-2448000 V_r sigma 453.506 -6.8 0.5 495.428 -6.5 0.5 496.450 1.4 0.7 448.385 -32.2 0.6 556.114 -2.2: 1.0 557.184 -36.4 1.0 558.156 -32.3 0.6 559.148 -20.5 0.6 561.166 -4.1 0.8 562.144 -5.5 0.8 563.143 -36.2 0.9 566.187 -12.2 0.4 567.135 -1.2 0.9 795.428 -23.4 0.6 807.487 -24.1 0.7 823.405 10.8 0.8 824.488 -13.6 0.9 825.478 -25.0 0.5 827.482 -7.7 0.4 830.498 -16.0 0.7 831.466 -24.5 0.7 832.443 -16.9 0.8 833.434 -7.8 0.5 834.428 -1.9 0.5 835.476 12.2 0.5 846.352 -2.2 0.4 848.437 -18.5 0.6 849.407 -24.6 0.5 850.380 -23.8 0.7 851.339 -10.5 0.4 854.313 -17.0 0.7 856.318 -18.6 0.5 857.372 -9.5 0.4 858.373 -3.5 0.6 We wish to thank Mr. O. Ugolnikov for his assistance during the observations. We are grateful to the administrations of the observatories for allocating observing time for this program and to the staff of the observatories for their help. N. A. GORYNYA N. N. SAMUS Institute for Astronomy, Russian Acad. Sci. 48, Pyatnitskaya Str., Moscow 109017, Russia T. R. IRSMAMBETOVA YU. V. KULAGIN A. S. RASTORGOUEV M. G. SMEKHOV A. A. TOKOVININ Sternberg Astronomical Institute 13, University Avenue, Moscow 119899, Russia References: Barnes, T. G. III., Moffet, T. J., Slovak, M. H., 1988, Astrophys. J. Suppl. 66, 43 [BIBCODE 1988ApJS...66...43B ] Gorynya, N. A., Irsmambetova, T. R., Rastorgouev, A. S., Samus, N. N., 1992, Soviet Astronomy Letters, in press [BIBCODE 1992SvAL...18..316G ] Joy, A. H., 1937, Astrophys. J., 86, 380 [BIBCODE 1937ApJ....86..363J ] Struve, O., 1945, Astrophys. J., 102, 232 [BIBCODE 1945ApJ...102..232S ] Szabados, L., 1991, Commun. Konkoly Obs., No. 96 [BIBCODE 1991CoKon..96..123S ] [CoKon No. 96] Tokovinin, A. A., 1987, Soviet Astronomy, 31, 98 [BIBCODE 1987SvA....31...98T ]