Circular No. 5058 Central Bureau for Astronomical Telegrams INTERNATIONAL ASTRONOMICAL UNION Postal Address: Central Bureau for Astronomical Telegrams Smithsonian Astrophysical Observatory, Cambridge, MA 02138, U.S.A. Telephone 617-495-7244/7440/7444 (for emergency use only) TWX 710-320-6842 ASTROGRAM CAM EASYLINK 62794505 MARSDEN or GREEN@CFA.BITNET MARSDEN or GREEN@CFAPS2.SPAN SUPERNOVA 1990S IN MCG -05-29-006 M. Hamuy, Cerro Tololo Interamerican Observatory; and J. Maza, Astronomy Department, University of Chile, report: "Roberto Antezana has discovered a supernova 7" west and 5" north of the nucleus of the spiral galaxy MCG -05-29-006 (ESO 440-G48). The supernova (estimated magnitude B = 15.5) was found on a 15-min 103a-O plate taken by Hamuy and L. Wells with the Curtis Schmidt telescope on July 22.046 UT. The SN is at R.A. = 12h02m58s.6, Decl. = -29 52'58" (equinox 1950.0). Confirmation was made by T. Williams (Rutgers University), who obtained UBVRI CCD images with the CTIO 0.9-m telescope on July 25, showing the SN to be very blue. A spectrum (range 630-950 nm) obtained on the same night by M. Phillips with the CTIO 4-m telescope shows a featureless continuum, along with narrow H-alpha and [N II] emission lines. These data do not allow a definitive classification, but it would appear most likely that this is a type-II supernova in an early stage of its evolution." UX ANTLIAE Observations by E. R. Minniti, Sante Fe, Argentina, telexed by L. A. Milone, Observatorio Astronomico, Universidad Nacional de Cordoba, indicate that this suspected R CrB-type variable is fading. Visual magnitude estimates by Minniti unless otherwise noted: May 21.0 UT, 11.2; June 9.0, 11.4; 16.0, 11.6; 19.0, 11.7; July 11.0, [12.7; 19.0, [13.0; 22.0, 14.0: (S. Paolantonio, Cordoba Observatory). Monitoring by Minniti since 1975 has revealed no brightness variations > 0.1-0.2 mag (normal mv = 11.3). NO OCCULTATION OF SAO 187435 BY TRITON L. Wasserman, Lowell Observatory, reports that, based on measurements of a plate obtained by A. Klemola with the Lick Observatory Astrograph, the proposed occultation of SAO 187435 by Triton (Neptune I) on 1990 Aug. 1 (Wasserman et al. 1990, A.J. 99, 732) will not occur. COMET TSUCHIYA-KIUCHI (1990i) Total visual magnitude estimates: July 16.73 UT, 10 (X.-m. Zhou, Bo Lo County, Xin Jiang province, China; independent discovery); 19.26, 8.8 (C. Spratt, Victoria, BC, 0.15-m reflector); 22.23, 8.7 (Spratt, 0.20-m reflector); 24.12, 8.9 (G. Kronk, Troy, IL, 0.33-m reflector). 1990 July 25 (5058) Daniel W. E. Green
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