Circular No. 3333 Central Bureau for Astronomical Telegrams INTERNATIONAL ASTRONOMICAL UNION Postal Address: Central Bureau for Astronomical Telegrams Smithsonian Astrophysical Observatory, Cambridge, MA 02138, U.S.A. TWX 710-320-6842 ASTROGRAM CAM Telephone 617-864-5758 mu SAGITTARII M. Plavec, Department of Astronomy, University of California at Los Angeles, writes: "The star mu Sgr (HD 166937, V ~ 3.86, B8Ia) has long been known to be a single-spectrum spectroscopic binary with a period of 180.45 days. Elvey (1938, Astrophys. J. 88, 110) observed a shallow partial eclipse of the B8 supergiant, with a duration of about 20 days and a maximum depth (in B) of ~ 0.14 magnitude. In 1978, using the spectrographs aboard the satellites IUE and Copernicus, R. S. Polidan and I detected a flux excess and some spectral lines in the region 1000-1400 A, presumably due to a hotter companion, of spectral type perhaps B0-3V. An eclipse of this companion was predicted for 1978 Sept. 11, and indeed Copernicus scans on Sept. 12-14 showed a considerably reduced flux in the region 1000-1200 A. Although the star has not been observed for many years, the old ephemeris therefore appears to be good enough to predict the next mid-eclipse of the companion for 1979 Mar. 10. Since this is the primary eclipse its depth in B may well be as much as 0.35 magnitude. The duration of the eclipse may be ~ 20 days." 1979 BA Y. Kozai, Tokyo Astronomical Observatory, telexes the following observation by E. Helin and K. Tomita at the Kiso Station: 1979 UT R. A. (1950) Decl. Mag. Feb. 19.46767 10 33.9 +27 16 17 This approximate position leads to a slight refinement (Incl. = 46o.2) of the elements on IAUC 3329 and the resulting ephemeris: 1979 ET R. A. (1950) Decl. Delta r Mag. Mar. 8 10 10.80 +39 29.3 0.841 1.741 17.3 13 10 04.85 +42 00.0 18 9 59.90 +44 00.4 0.944 1.767 17.7 23 9 56.12 +45 34.2 28 9 53.63 +46 44.9 1.063 1.792 18.1 Apr. 2 9 52.45 +47 36.2 7 9 52.57 +48 11.5 1.191 1.818 18.4 12 9 53.91 +48 33.3 17 9 56.36 +48 43.9 1.322 1.843 18.7 1979 February 26 (3333) Brian G. Marsden
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