Circular No. 4086 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 617-495-7244/7440/7444 PERIODIC COMET GICLAS (1985g) This comet has been recovered by E. Everhart on an exposure by J. Briggs and by C.-Y. Shao on exposures by G. Schwartz: 1985 UT R.A. (1950.0) Decl. m1 Observer June 22.38646 0 53 11.05 - 0 36 55.6 20 Everhart July 18.30242 1 43 07.71 + 2 36 51.6 18 Shao 21.30067 1 48 45.37 + 2 55 06.1 18 " E. Everhart (Chamberlin Observatory field station, near Denver). 0.4-m reflector. Weak image, unconfirmed at the time. C.-Y. Shao (Oak Ridge Observatory). 1.5-m reflector. Plates very dark; inkdot measured on July 18. The comet's image is strongly condensed, possibly even stellar in appearance. The above positions show that the prediction by S. Nakano on MPC 9362 (elements on MPC 8289) requires correction by Delta-T = -0.66 day. An improved ephemeris follows: 1985 ET R.A. (1950.0) Decl. p r m1 July 14 1 34.96 + 2 08.9 1.714 1.966 18.1 24 1 53.77 + 3 11.0 Aug. 3 2 11.94 + 4 01.6 1.487 1.911 17.7 13 2 29.17 + 4 39.5 23 2 45.07 + 5 03.7 1.284 1.871 17.3 Sept. 2 2 59.17 + 5 14.2 12 3 10.98 + 5 11.6 1.112 1.846 16.9 22 3 19.94 + 4 57.6 Oct. 2 3 25.61 + 4 36.0 0.980 1.838 16.6 12 3 27.73 + 4 11.7 22 3 26.38 + 3 51.3 0.901 1.847 16.4 CPD -58 2721 J. S. Drilling, Louisiana State University; U. Heber, Universitat Kiel; and C. S. Jeffery, St. Andrews University, report that the extreme helium star CPD -58 2721 (Drilling 1980, Ap.J. 242, L43) has changed in radial velocity by 138 +/- 10 km/s between 1983 May 30.1 and 1985 Apr. 9.1 UT. This result is based on high- resolution spectra obtained at Cerro Tololo, the European Southern Observatory and with the Anglo-Australian Telescope, and it suggests that CPD -58 2721 is an H-deficient binary like nu Sgr and KS Per. 1985 July 23 (4086) Brian G. Marsden
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