Circular No. 3263 Central Bureau for Astronomical Telegrams INTERNATIONAL ASTRONOMICAL UNION Postal Address: Central Bureau for Astronomical Telegrams Smithsonian Astrophysical Observatory, Cambridge, MA 02138, U.S.A. TWX 710-320-6842 ASTROGRAM CAM Telephone 617-864-5758 NOVA CYGNI 1978 Peter L. Collins, Mount Hopkins Observatory, reports the discovery of a nova on Sept. 10.24 UT at the position R.A. = 21h40m.6, Decl. = +43o48' (equinox 1950.0). Several visual magnitude estimates by the discoverer during Sept. 10.31-10.50 UT gave 6.9-7.0. From a visual inspection of the same region the previous night it was concluded that the object was probably then fainter than magnitude 9. C.-Y. Shao, Center for Astrophysics, has measured the following precise position from a plate (somewhat overexposed) obtained by G. Schwartz with the 41-cm Metcalf astrograph at Harvard Observatory's Agassiz Station: 1978 UT R. A. (1950) Decl. mpg Sept. 10.33785 21 40 38.28 +43 48 09.8 6.8 The object was evidently fainter than magnitude 14 when a Harvard patrol plate was taken on Sept. 2. A cursory inspection of the Palomar Sky Survey prints reveals a possible candidate for the prenova near the magnitude limit. Further visual magnitude estimates: Sept. 10.50 UT, 6.6 (M. Hiraga, Dazaifu, Fukuoka; independent discovery); 11.0, 6.3 (D. Proust and M. Verdenet, Meudon Observatory; independent discovery); 11.07, 6.4 (T. Bretl, Overland Park, Kansas); 11.13, 6.3 (J. Morgan, Prescott, Arizona); 11.16, 6.6 (C. Hurless, Lima, Ohio); 11.17, 6.4 (R. Annal, Barstow, California); 11.19, 6.6 (E. Mayer, Barberton, Ohio); 11.28, 6.7 (P. L. Collins, Mount Hopkins Observatory). PERIODIC COMET HANEDA-CAMPOS (1978j) Shao has also measured the following precise positions from exposures by Schwartz with the 41-cm Metcalf astrograph: 1978 UT R. A. (1950) Decl. Sept. 6.20498 20 58 27.85 -32 03 13.6 8.16787 21 02 33.40 -33 11 43.8 A visual estimate by Collins on Sept. 7.22 UT (20-cm reflector) put the comet at magnitude 10.2. 1978 September 11 (3263) Brian G. Marsden
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