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Circular No. 7511 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) SUPERNOVA 2000dw IN UGC 11955 Y. L. Qiu and J. Y. Hu, Beijing Astronomical Observatory (BAO), on behalf of the BAO Supernova Survey, report the discovery of an apparent supernova (mag about 17.5) in unfiltered images taken on Oct. 17.5 and 20.6 UT with the BAO 0.6-m telescope. The new object was confirmed by W. D. Li, University of California at Berkeley, on unfiltered images taken on Oct. 19.2 with the 0.8-m Katzman Automatic Imaging Telescope. SN 2000dw is located at R.A. = 22h13m49s.06, Decl. = +39o14'15".1 (equinox 2000.0), which is 1".5 east and 3".3 north of the center of UGC 11955. Photometry is difficult, as the object is very close to the nucleus of the parent galaxy. Unfiltered BAO images taken on July 12 (limiting mag about 19.0) showed no star at the position of the new object. SUPERNOVAE 2000ds, 2000dt, 2000du, 2000dv A. V. Filippenko and R. Chornock, University of California at Berkeley, communicate: "Inspection of CCD spectra (range 330-1000 nm) of SN 2000dt (IAUC 7508), obtained on Oct. 24 UT with the Shane 3-m reflector at Lick Observatory, reveal that the object is probably of type Ib. He I absorption lines are present, but there is also an unidentified line at rest wavelength 622 nm (possibly blueshifted C II 658 nm, or perhaps H-alpha, though the corresponding H-beta line seems absent). SN 2000dv (IAUC 7509) is also a type-Ib supernova, about 3 months past maximum brightness; it is starting to enter the nebular phase, but He I absorption is still present. SN 2000ds (IAUC 7507) is an even older type-Ib (or -Ic) supernova, perhaps 4 to 7 months past maximum; we prefer the type-Ib classification because the [Ca II] 732-nm emission has FWHM approximately 5000 km/s, most consistent with type-Ib supernovae (Filippenko et al. 1995, Ap.J. 450, L11; Matheson et al. 2001, A.J., in press). SN 2000du (IAUC 7509) is a normal type-II supernova; H-alpha exhibits a classic P-Cyg profile." COMET C/1999 Y1 (LINEAR) Total visual magnitude estimates (L = reflector): Aug. 5.00 UT, 13.7 (M. Meyer, Frauenstein, Germany, 0.25-m L); 26.30, 14.2 (A. Hale, Cloudcroft, NM, 0.41-m L); Sept. 8.90, 13.7 (W. Hasubick, Buchloe, Germany, 0.44-m L); Oct. 6.01, 12.9 (G. Comello, Roden, The Netherlands, 0.31-m L); 17.79, 12.6 (R. J. Bouma, Groningen, The Netherlands, 0.25-m L); 23.76, 12.1 (M. Lehky, Hradec Kralove, Czech Rep., 0.42-m L). (C) Copyright 2000 CBAT 2000 October 24 (7511) Daniel W. E. Green
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