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Circular No. 6753 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) BMARSDEN@CFA.HARVARD.EDU or DGREEN@CFA.HARVARD.EDU (science) URL http://cfa-www.harvard.edu/iau/cbat.html Phone 617-495-7244/7440/7444 (for emergency use only) COMET C/1997 T1 (UTSUNOMIYA) Preliminary parabolic orbital elements by S. Nakano, Sumoto, Japan, from 46 observations (Oct. 5-6). T = 1997 Dec. 10.836 TT Peri. = 96.950 Node = 53.942 2000.0 q = 1.34933 AU Incl. = 128.182 1997 TT R. A. (2000) Decl. Delta r Elong. Phase m1 Oct. 4 23 16.2 +72 36.5 1.033 1.670 110.5 34.1 10.3 5 22 52.2 +72 14.2 1.026 1.662 110.3 34.4 10.3 6 22 29.2 +71 40.3 1.019 1.654 110.0 34.6 10.2 7 22 07.5 +70 55.6 1.014 1.646 109.6 34.9 10.2 8 21 47.5 +70 01.1 1.011 1.638 109.2 35.2 10.2 9 21 29.33 +68 58.2 1.008 1.630 108.6 35.5 10.1 10 21 12.89 +67 47.9 1.006 1.622 108.0 35.8 10.1 11 20 58.17 +66 31.6 1.006 1.614 107.3 36.2 10.1 12 20 45.02 +65 10.4 1.006 1.607 106.6 36.5 10.1 13 20 33.32 +63 45.3 1.008 1.599 105.7 36.9 10.1 14 20 22.90 +62 17.2 1.011 1.591 104.8 37.3 10.0 15 20 13.62 +60 46.9 1.015 1.584 103.9 37.7 10.0 16 20 05.35 +59 15.2 1.019 1.577 102.9 38.1 10.0 17 19 57.96 +57 42.7 1.025 1.569 101.8 38.4 10.0 18 19 51.34 +56 09.9 1.032 1.562 100.7 38.8 10.0 19 19 45.41 +54 37.2 1.040 1.555 99.6 39.2 10.0 20 19 40.07 +53 05.0 1.049 1.548 98.4 39.5 10.0 21 19 35.27 +51 33.7 1.058 1.541 97.2 39.9 10.0 22 19 30.92 +50 03.6 1.069 1.534 95.9 40.2 10.0 23 19 26.99 +48 34.8 1.080 1.527 94.7 40.5 10.0 24 19 23.43 +47 07.7 1.092 1.521 93.4 40.8 10.0 25 19 20.19 +45 42.3 1.105 1.514 92.1 41.0 10.0 26 19 17.24 +44 18.7 1.118 1.508 90.9 41.3 10.0 27 19 14.56 +42 57.1 1.133 1.501 89.6 41.5 10.0 28 19 12.10 +41 37.5 1.147 1.495 88.3 41.6 10.0 29 19 09.86 +40 20.0 1.163 1.489 87.0 41.8 10.1 SUPERNOVA 1997dg IN ANONYMOUS GALAXY L. Wang, C. Pulliam, and J. C. Wheeler, University of Texas, report: "A spectrum of SN 1997dg was obtained on Oct. 1.3 UT at the 2.7-m telescope (+ LCS) of the McDonald Observatory. We confirm that this is a type-Ia supernova a few days past maximum (cf. IAUC 6749). The redshift of the host galaxy is about 0.034, assuming a Ca II (H and K) expansion velocity for the ejecta of 12 000 km/s." (C) Copyright 1997 CBAT 1997 October 6 (6753) Daniel W. E. Green
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