Circular No. 3848 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 COMET CERNIS (1983l) Further precise positions have been reported as follows: 1983 UT R.A. (1950.0) Decl. m1 Observer July 25.77893 2 42 19.12 +10 21 51.5 13 Seki 26.75648 2 42 08.81 +10 09 10.2 Gilmore 26.76215 2 42 08.76 +10 09 06.0 " T. Seki (Kochi Observatory, Geisei Station). A. C. Gilmore (Mt. John Observatory). Measurer: P. M. Kilmartin. Improved parabolic elements from observations July 21-26: T = 1983 July 24.196 ET Peri. = 186.918 Node = 208.877 1950.0 q = 3.31349 AU Incl. = 134.808 1983 ET R.A. (1950.0) Decl. p r m1 Aug. 4 2 39.90 + 8 12.0 14 2 35.00 + 5 23.8 2.959 3.319 10.6 24 2 27.35 + 2 03.9 Sept. 3 2 16.62 - 1 49.0 2.633 3.336 10.3 13 2 02.64 - 6 10.8 23 1 45.60 -10 49.9 2.450 3.363 10.2 epsilon AURIGAE M. Parthasarathy and D. L. Lambert, McDonald Observatory, report: " Observations of epsilon Aur during totality near zero phase show a significant decrease in the strength of the K 770-nm resonance line: W-lambda was 0.055 nm during 1982 Dec.-1983 Mar., 0.040 nm during Apr.-May and 0.024 nm during July. The Na D lines also decreased in strength, their strength now being similar to that before the eclipse. The H-alpha line is broad, and the emission in the wings has disappeared. These observations suggest that the neutral gas is mostly confined to the outer regions of the eclipsing object." GK PERSEI J. Mattei, AAVSO, communicates the following additional visual magnitude estimates (cf. IAUC 3840): July 21.30 UT, 11.9 (J. Bortle, Stormville, NY); 23.30, 11.5 (C. Scovil, Stamford, CT); 25.30, 11.6 (Bortle). 1983 August 5 (3848) Brian G. Marsden
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