Circular No. 3031 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 Telex: 921428 Telephone: (617) 864-5758 V1500 CYGNI P. Tempesti, Collurania Observatory, writes: "Photoelectric observations performed with the Teramo refractor on 1976 Dec. 13 and covering a complete cycle of the 3-hr short period light variation show an amplitude of 0.52 magnitude in V, much greater than ever reported before. The period appears to have shortened from 0d.141 at the time of early decline to 0d.130,confirming the gradual decrease found by Semeniuk et al. (1976, Inf. Bull. Variable Stars No. 1157). Moreover, there is an indication of light modulation of shorter period and mean amplitude about 0.06 magnitude. The mean V magnitude on 1976 Dec. 13.8 UT was 12.85 +/- 0.03." Recent visual magnitude estimates: Jan. 1.98 UT, 12.4 (J. Bortle, Brooks Observatory); 11.08, 12.4 (S. O'Meara, Harvard College Observatory); 18.06, 12.4 (O'Meara); 21.01, 12.5 (Bortle). AQUILA X-1 S. S. Holt and L. J. Kaluzienski, Laboratory for High Energy Astrophysics, Goddard Space Flight Center, report the confirmation of flaring activity in Aql X-1 = 3U 1908+00 from the Ariel 5 all-sky monitor. Following a private communication from M. Watson, University of Leicester, that the Ariel 5 sky survey instrument showed an increase in intensity over a few days up to a level of 0.15 times the Crab on Jan. 9, the all-sky monitor data were interrogated from the appearance of Aql X-1 at the edge of the experiment field of view on Jan. 12. Data obtained during Jan 12-15 are consistent with a constant source intensity of 0.3 times the Crab, at least three times less than the extended maxima of the flaring episodes of June 1975 and June 1976 (cf. IAUC 2788, 2965). PERIODIC COMET SCHWASSMANN-WACHMANN 1 The following precise positions have been reported: 1976 UT R. A. (1950) Decl. m1 Observer Oct. 30.62222 3 12 54.42 +29 22 20.8 11.5 Seki 31.75833 3 12 19.4 +29 20 44 11.5 " Nov. 29.62826 2 57 24.62 +28 18 08.7 14.5 " Dec. 19.81321 2 49 46.00 +27 22 24.5 12.7 Mrkos 19.82756 2 49 45.88 +27 22 23.4 " 20.77826 2 49 30.48 +27 19 51.3 12.7 " 20.78914 2 49 30.26 +27 19 50.5 " 21.71711 2 49 16.18 +27 17 25.0 12.9 " 21.73134 2 49 15.82 +27 17 23.0 " 22.77201 2 49 00.34 +27 14 36.7 12.7 " 22.78347 2 49 00.12 +27 14 35.8 " 25.74153 2 48 21.00 +27 06 58.1 12.9 " 27.75478 2 47 57.75 +27 02 01.1 13.0 " T. Seki (Kochi Observatory, Geisei Station). From Orient. Astron. Assoc. Comet Bull. No. 139. A. Mrkos (Klet Observatory). J. Bortle, Brooks Observatory, provides further visual magnitude estimates (32-cm reflector): 1976 Dec. 24.99 UT, 12.4 (stellar nucleus 14.1); 27.17, 12.4 (no nucleus); 1977 Jan. 9.00, [13.5. COMET HARLAN (1976g) Further precise positions have been reported as follows: 1976 UT R. A. (1950) Decl. m2 Observer July 19.12279 13 16 42.66 +21 36 05.7 Shao Sept.18.31962 14 44 42.48 - 7 11 35.4 14.7 Gilmore Oct. 24.35391 16 09 22.75 -23 46 20.6 " C. Y. Shao (Harvard College Observatory, Agassiz Station). A. C. Gilmore (Carter Observatory). 41-cm reflector. Measurer: P. M. Kilmartin. Oct. 24 image very diffuse. COMET BRADFIELD (1976d) The following precise positions were obtained by C. Torres at the University of Chile's Cerro El Roble Station: 1976 UT R. A. (1950) Decl. Mar. 27.06248 4 14 22.80 -14 27 44.8 28.03114 4 18 51.90 -13 03 58.4 OBSERVATIONS OF MINOR PLANETS The following precise positions of 1963 UA and 1975 YA were obtained by E. Roemer and L. M. Vaughn with the Steward Observatory's 229-cm reflector, Kitt Peak. Measurer: C. D. Vesely. Object 1976 UT R. A. (1950) Decl. Mag. 1963 UA June 26.37216 23 29 06.92 +11 33 04.1 19.6 26.39259 23 29 09.82 +11 33 26.1 27.40851 23 31 30.38 +11 50 52.3 19.7 1975 YA June 25.29840 18 41 09.55 -32 01 25.1 25.30887 18 41 04.84 -32 02 36.0 1977 January 26 (3031) Brian G. Marsden
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