Circular No. 2808 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 POSSIBLE NOVA IN SAGITTARIUS Dr. K. Osawa, Director of the Tokyo Astronomical Observatory, communicates the following visual magnitude estimates by Yoshiyuki (not Yoshikuyi, as was given on IAUC 2805) Kuwano: July 24.597 UT, 10.2; 25.572, 10.1; 26.623, 10.3. The comparison star was SAO 185987 (CoD -28 13895). On July 8 the possible nova was fainter than magnitude 11. Mr. C. Scovil, Stamford Museum, provides the following photovisual magnitude estimate: July 27.16 UT, 11.0 +/- 0.5. POSSIBLE COMET ANTAL Mr. M. Antal, Skalnate Pleso Observatory, reports the possible discovery of a comet, as follows: 1975 UT R. A. (1950) Decl. m1 July 8.93611 18 05.2 -21 05 14 The object was diffuse, without condensation or nucleus. The daily motion was about 1o in p.a. 60o or 240o. MX1401-45 D. Hearn, Massachusetts Institute of Technology, reports that the SAS-3 group has discovered a source of soft x-rays at R.A. = 14h01m +/- 1m, Decl. = -45o.2 +/- 0o.4 (equinox 1950.0). The source, discovered on July 15, appears to be smaller than 1o in extent. It is detected most strongly in the 0.1 to 0.28 keV energy band, at a level of about 10 percent of the total Cygnus Loop intensity in that band. A weak signal present in the 0.4 to 0.7 keV band indicates a spectral temperature of 3 x 10**6 K or less. A1524-61 M. Watson, X-Ray Astronomy Group, University of Leicester, sends the following improved position, derived from Ariel 5 Sky Survey observations, of the transient x-ray source A1524-61 (= TrA X-1) mentioned on IAUC 2729: R.A. =15h23m32s +/- 5s, Decl. = -61o49'.4 +/- 1'.2 (equinox 1950.0). 1975 July 29 (2808) Brian G. Marsden
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