Circular No. 4787 Central Bureau for Astronomical Telegrams INTERNATIONAL ASTRONOMICAL UNION Postal Address: Central Bureau for Astronomical Telegrams Smithsonian Astrophysical Observatory, Cambridge, MA 02138, U.S.A. Telephone 617-495-7244/7440/7444 (for emergency use only) TWX 710-320-6842 ASTROGRAM CAM EASYLINK 62794505 MARSDEN or GREEN@CFA.BITNET MARSDEN or GREEN@CFAPS2.SPAN PERIODIC COMET DU TOIT-NEUJMIN-DELPORTE (1989l) J. Gibson reports that he has recovered this comet with the 1.5-m reflector + CCD at Palomar as follows: 1989 UT R.A. (1950) Decl. m1 May 22.26339 15 20 16.69 -14 21 05.2 18.5 22.26670 15 20 16.46 -14 21 04.1 22.26992 15 20 16.35 -14 21 03.6 23.29112 15 19 24.01 -14 16 14.0 23.29778 15 19 23.62 -14 16 11.8 23.31285 15 19 22.84 -14 16 07.2 There is a stellar nucleus and perhaps some hint of a faint coma. The indicated correction to the prediction on MPC 12135 (ephemeris on MPC 14036) is delta T = +0.03 day. PERIODIC COMET KOPFF (1988k) K. Jockers, Max-Planck-Institut fur Aeronomie, Katlenburg-Lindau; and G. Chernova, Institut Astrofiziki, Dushanbe, report: "CCD photometry of P/Kopff has been performed with the 1-m reflector at the Hoher List Observatory using a focal reducer and wide-band filters. During May 6.88-6.94 UT the total magnitude was determined to be 18.5 +/- 0.3 at an effective wavelength of 434 nm and 16.6 +/- 0.3 at 680 nm. The comet is significantly redder than the sun. At the focal-reducer scale of 1".7 per pixel evidence for an extended coma is at best marginal." V404 CYGNI S. Okamura and W. Tanaka, Kiso Observatory, have identified the optical counterpart of GS 2023+338 at B = 15 +/- 1 on a plate taken with the 1.05-m Schmidt on May 28 and give the position as R.A. = 20 22 06.30 +/- 0.03, Decl. = +33 42'16".7 +/- 0".4 (equinox 1950.0). They estimate from the Palomar Sky Survey charts that B is approximately 21, R approximately 18.5. Visual magnitude estimates by P. Schmeer, Bischmisheim, West Germany: May 28.04 UT, 11.9; 30.02, 12.4; June 1.03, 13.6. 1989 June 1 (4787) Brian G. Marsden
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