Circular No. 4647 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 617-495-7244/7440/7444 MARSDEN or GREEN@CFA.BITNET MARSDEN or GREEN@CFAPS2.SPAN PERIODIC COMET KOPFF (1988k) E. M. Alvarez and M. J. S. Belton, National Optical Astronomy Observatories; and K. J. Meech, Institute for Astronomy, University of Hawaii, report their recovery of P/Kopff with the University of Hawaii 2.2-m telescope on Mauna Kea. The object is centrally condensed without any obvious coma; magnitude R ~ 21. 1988 UT R.A. (1950) Decl. Feb. 11.24033 8 42 20.98 +19 20 10.5 11.24829 8 42 20.87 +19 20 10.9 11.25586 8 42 20.55 +19 20 12.8 Mar. 19.22941 8 22 29.05 +20 41 09.9 19.24510 8 22 28.86 +20 41 09.7 19.25324 8 22 28.72 +20 41 10.3 20.23675 8 22 11.97 +20 42 17.4 20.25008 8 22 11.78 +20 42 18.6 20.25610 8 22 11.59 +20 42 19.0 22.22907 8 21 41.23 +20 44 19.0 22.24080 8 21 41.02 +20 44 18.7 SUPERNOVA 1935C IN NGC 1511 S. van den Bergh, Dominion Astrophysical Observatory; and M. L. Hazen, Center for Astrophysics, report that HV 11970, mentioned by E. H. Boyce (1943, Harvard Bull. No. 917) as a possible nova associated with the LMC and sometimes known as Nova Hydri 1935, is rather definitely a supernova in NGC 1511 (R.A. = 3h59m.3, Decl. = -67D46', equinox 1950.0), an alternative also suggested by Boyce. The object reached its observed maximum of mpg = 12.5 on 1935 Sept. 19 and was located about 55" east and 8" south of the galaxy's nucleus. COMET MACHHOLZ (1988j) L. Lebofsky, P. Owensby, and W. Golisch report broadband infrared observations from the NASA Infrared Telescope Facility on Mauna Kea on Aug. 23.7 UT. Through a 7".8-diameter aperture, the monochromatic magnitudes were: J = 12.07 +/- 0.01, H = 11.57 +/- 0.01, K = 11.58 +/- 0.01, N = 2.61 +/- 0.02, Q = 0.90 +/- 0.20. 1988 August 25 (4647) Daniel W. E. Green
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