Circular No. 2254 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 NOVA CYGNI 1970 Dr. L. Kohoutek, Hamburg Observatory, Bergedorf, communicates the following magnitudes (referred to the photoelectric sequence in NGC 6913), estimated from plates taken with the 80-cm f/3 Schmidt before the announcement of the nova's discovery: 1969/70 UT B 1970 UT B Nov. 5.74 18: May 24.0217 9.4 May 2.04 18: June 9.0178 10.6 On the first two plates the nova is near the limit. On five other plates, of limiting magnitude 17.5 to 18.0, taken between August 1969 and April 1970 the prenova is invisible. On the Palomar Sky Atlas prints (July 1951, O-288 and O-279) the prenova was identified as a star of magnitude B = 18.1; it lies 8".6 northwest of a fainter star of about B = 18.4. Using the computer program by Dieckvoss the nova's position was determined to be: R.A. = 20h50m46s.364 +/- 0s.009 Decl. = +35o48'02".04 +/- 0".04 (1950) Mr. C. Y. Shao, Harvard College Observatory, provides the following measures, the photographic ones from plates exposed at the Agassiz station by M. Mattei. The photoelectric observation, made under poor sky conditions, is referred to HBV 475 sequence stars. 1970 UT mpg V B - V May 30.263 9.8 June 15.292 10.95 -0.08 15.342 10.8 PERIODIC COMET D'ARREST (1970d) Mr. T. Urata, Fujikan Center Observatory, Nihondaira, Shimizu, Shizuoka, writes that he observed this comet visually on June 8.760 UT, using a 20-cm refractor, 50x. The total visual magnitude was 11, the diameter 3', and there was no central condensation; the seeing was poor. Precise positions of this comet are of particular importance in view of the possibility that a space probe will be sent to the comet in 1976. 1970 June 18 (2254) Brian G. Marsden
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