Circular No. 2978 Central Bureau for Astronomical Telegrams INTERNATIONAL ASTRONOMICAL UNION Postal Address: Central Bureau for Astronomical Telegrams Smithsonian Astrophysical Observatory, Cambridge, MA 02138, U.S.A. Cable Address: SATELLITES, NEWYORK Western Union: RAPID SATELLITE CAMBMASS NEW MIRA VARIABLE IN SCUTUM Cablegrams received from K. Osawa, Tokyo Observatory, report the discovery, by Y. Kuwano, Hita, Oita, of a variable stellar object at R.A. = 18h24m.1, Decl. = -14o42' (equinox 1950.0). The brightness was given as mpv = 11.0 on June 28.68 UT and mv = 12.2 on July 14.59. The Central Bureau relayed word of this "possible nova" to telegram subscribers. D. Hoffleit, Maria Mitchell Observatory, informs us that the object appears on five plates taken between June 4 and July 3 UT, some fading being evident during this interval. The star was slightly fainter on a plate taken on 1920 Oct. 14, appreciably fainter on five other plates taken during the past half century and invisible on more than 30 more plates of the field. She suggests that the star is a Mira variable of period about 383 days and notes that at minimum the star is certainly fainter than magnitude 14. UU SAGITAE E. L. Wright and W. Liller, Center for Astrophysics, report an improved period of 11h09m41s.95 +/- 0s.02 based on eight minima found from Harvard plates between 1927 and 1946 and the time of mid-eclipse given on IAUC 2974. JUPITER XIII (LEDA) E. Roemer provides the following precise positions, obtained with the Steward Observatory's 229-cm reflector. L. M. Vaughn assisted. Measurer: C. D. Vesely. 1975 UT R. A. (1950) Decl. Nov. 1.22766 1 08 07.69 + 5 04 12.7 1.27176 1 08 06.29 + 5 04 03.5 EDITORIAL NOTICE Contributors are advised that during the Director's absence abroad for the next six weeks only the most urgent communications will be reported in these Circulars. Such communications should generally be telegraphed to the Central Bureau; the telephone number (617) 864-5758 will not be operational during this period. 1976 July 23 (2978) Brian G. Marsden
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