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Circular No. 8692 Central Bureau for Astronomical Telegrams INTERNATIONAL ASTRONOMICAL UNION Mailstop 18, Smithsonian Astrophysical Observatory, Cambridge, MA 02138, U.S.A. IAUSUBS@CFA.HARVARD.EDU or FAX 617-495-7231 (subscriptions) CBAT@CFA.HARVARD.EDU (science) URL http://cfa-www.harvard.edu/iau/cbat.html ISSN 0081-0304 Phone 617-495-7440/7244/7444 (for emergency use only) COMET C/2006 F2 (CHRISTENSEN) E. J. Christensen reports the discovery of a comet on unfiltered CCD images taken with the 1.5-m reflector in the course of the Mt. Lemmon Survey (discovery observation tabulated below). The Mar. 23 images show a diffuse, round 8" coma and no tail in four co-added 30-s images. Four co-added 60-s images in average seeing taken on Mar. 24.3 UT show a 10" moderately condensed coma, slightly elongated toward p.a. 320 deg. 2006 UT R.A. (2000) Decl. Mag. Mar. 23.32673 12 36 46.72 - 3 57 46.6 19.7 The available astrometry (including prediscovery Spacewatch observations from Feb. 27), the following preliminary orbital elements, and an ephemeris appear on MPEC 2006-F29. T = 2006 Mar. 17.736 TT Peri. = 179.204 e = 0.65377 Node = 8.258 2000.0 q = 4.28917 AU Incl. = 20.413 a = 12.38814 AU n = 0.022604 P = 43.6 years COMET 73P/SCHWASSMANN-WACHMANN The components 'H', 'J', and L (mentioned on IAUC 8685 on Mar. 8) were observed by P. Birtwhistle (Great Shefford, Berkshire, England) on Mar. 23.1 UT and by E. J. Christensen at Mt. Lemmon on Mar. 23.5. Birtwhistle gave the magnitudes as 18.9, 19.9, and 21.0, adding that component 'H' had a coma of diameter 9" and a tail 40" long in p.a. 255 deg, that component 'J' had a coma of diameter 9" and a tail 20" long in p.a. 230 deg, and that component 'L' had a very diffuse coma of diameter 5" and a possible tail 15" long in p.a. 245 deg. Neither observer recorded component 'K', but both observers independently reported two new components, designated 'M' and 'N', estimated by Birtwhistle at mag 20.8 and 21.4, respectively, the former having a diameter of no more than 4" and no tail, and the latter having a stellar head and a faint tail 70" (possibly up to 90") long in p.a. 255 deg. The astrometric observations are provided on MPEC 2006-F22. The new components 'M' and 'N' are in the vicinity of component 'H' and, using the earlier orbit (MPEC 2006-B27) for component 'B' with perihelion time adjusted as before, they correspond to T = 2006 June 8.28 and 8.30 TT, respectively, although component 'N' lies perhaps 40" north of the line of variation. (C) Copyright 2006 CBAT 2006 March 24 (8692) Daniel W. E. Green
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