Circular No. 2972 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 HR 1099 M. Ryle, Cavendish Laboratory, reports that observations with the 5-km telescope reveal HR 1099 to be a variable radio source, as suggested by Landis and Hall (1976, Inf. Bull. Variable Stars No. 1113), who note its resemblance to UX Ari = HD 21242. A source within 0s.01 in R.A. of HR 1099 has varied in flux density between 20 and 60 mJy (at 5 GHz) during the past month, peaking on June 30. OPTICAL CANDIDATES FOR X-RAY SOURCES N. E. Kurochkin, Sternberg Astronomical Institute, proposes CSVS 4693 (R.A. = 19h25m44s, Decl. = +42o53'.2, equinox 1900.0; Belyavskij 1936, Pulkovo Obs. Circ. No. 19) as the optical counterpart of 3U 1921+43. Moscow plates during 1949-1970 show nonperiodic variations between mpg 13.5 and 17 over intervals of a few days. H. Pedersen, University of Aarhus, suggests the identification HR 3089 = 3U 0750-49. Observations of this He-strong B-type star at the European Southern Observatory in January and February show He variability with a period of 1.3295 +/- 0.0025 days. PERIODIC COMET D'ARREST (1976e) In response to requests we give here the orbital elements from which the ephemeris on IAUC 2964 was derived; and the ephemeris is tabulated at a 1-day interval during August. T = 1976 Aug. 12.8727 ET Epoch = 1976 Aug. 10.0 ET Peri. = 178.9266 e = 0.656147 Node = 141.3528 1950.0 a = 3.385158 AU Incl. = 16.6901 n = 0.1582471 q = 1.163996 AU P = 6.228 years 1976 ET R. A. (1950) Decl. 1976 ET R. A. (1950) Decl. Aug. 1 20 27.57 + 7 29.7 Aug. 16 22 01.32 -16 59.7 2 20 32.69 + 6 11.7 17 22 08.37 -18 40.7 3 20 38.00 + 4 49.6 18 22 15.40 -20 18.9 4 20 43.49 + 3 23.4 19 22 22.42 -21 53.6 5 20 49.18 + 1 53.3 20 22 29.38 -23 24.5 6 20 55.04 + 0 19.6 21 22 36.27 -24 51.3 7 21 01.07 - 1 17.5 22 22 43.07 -26 13.8 8 21 07.28 - 2 57.5 23 22 49.76 -27 31.8 9 21 13.64 - 4 40.1 24 22 56.32 -28 45.1 10 21 20.14 - 6 24.7 25 23 02.73 -29 53.9 11 21 26.78 - 8 10.7 26 23 08.99 -30 58.1 12 21 33.53 - 9 57,5 27 23 15.08 -31 57.8 13 21 40.38 -11 44.4 28 23 20.99 -32 53.1 14 21 47.31 -13 30.9 29 23 26.72 -33 44.2 15 21 54.29 -15 16.2 30 23 32.25 -34 31.3 PERIODIC COMET WOLF (1975f) E. Roemer provides the following precise positions: 1976 UT R. A. (1950) Decl. Note Aug. 8.23520 20 56 56.33 +22 14 38.8 1 8.27944 20 56 54.64 +22 14 27.5 1 Sept. 9.34215 20 41 18.74 +17 21 09.3 1 Oct. 7.15318 20 44 26.09 +10 59 59.2 1 Dec. 6.08403 21 48 27.32 + 2 14 32.2 2 6.12917 21 48 31.40 + 2 14 23.3 2 Note 1. Steward Observatory's 229-cm reflector, Kitt Peak. R. A. McCallister assisted on Aug. 8 and Sept. 9, M. Daniel assisted on Oct. 7. Measurer: C. C. McCarthy. Note 2. Lunar and Planetary Laboratory's 154-cm reflector, Catalina Station. Images weak. Measurer: C. D. Vesely. PERIODIC COMET ENCKE Continuation to the ephemeris on IAUC 2779: 1976 ET R. A. (1950) Decl. Delta r m2 July 21 0 11.02 + 5 25.7 3.235 3.754 21.4 31 0 07.94 + 5 26.4 Aug. 10 0 02.84 + 5 14.8 2.905 3.684 21.0 20 23 55.73 + 4 50.1 30 23 46.75 + 4 12.0 2.655 3.607 20.6 Sept. 9 23 36.33 + 3 22.0 19 23 25.06 + 2 22.9 2.522 3.522 20.3 29 23 13.73 + 1 19.1 Oct. 9 23 03.17 + 0 15.8 2.521 3.429 20.4 19 22 54.07 - 0 42.1 29 22 46.96 - 1 30.6 2.634 3.328 20.6 Nov. 8 22 42.12 - 2 07.3 18 22 39.61 - 2 30.9 2.818 3.219 20.8 28 22 39.36 - 2 41.1 Dec. 8 22 41.19 - 2 38.4 3.023 3.100 20.9 18 22 44.89 - 2 23.5 28 22 50.26 - 1 57.1 3.210 2.971 20.9 m2 = 15.5 + 5 log Delta + 5 log r + 0.03 (phase angle) 1976 July 12 (2972) Brian G. Marsden
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