Circular No. 4195 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 QSO 0716+332 B. Wills, Department of Astronomy, University of Texas, Austin, reports a visual-light outburst of this radio source (1950.0 position from University of Texas Radio Astronomy Observatory Sky Survey, +/- 1" : R.A. = 7h16m04.5s, Decl. = +33deg12'42"), as indicated by the following magnitudes: 19 (Palomar Sky Survey photo); 1981 Dec.- 1985 Feb. (one or more occasions), 20 or fainter; 1986 Feb. 6, ~ 17 (A. Crotts, McDonald Obs.); Mar. 13, 15.5 (D. Wills, McDonald Observatory). The spectrum is featureless except for a probable absorption doublet near 361.9 nm. A finding chart was published by Condon et al. (1979, A.J. 84, 149). omega ORIONIS D. P. Hayes, Astronomy Department, Columbia University, writes that the Be star omega Ori (HD 37490) recently displayed a large increase in linear polarization. On Jan. 29, the star's intrinsic polarization was 0.0 percent, but by Mar. 16 it had increased to a value of 0.63 percent. Polarization observations of this star will continue through mid-April. PERIODIC COMET CIFFREO (1985p) Ephemeris continuation (cf. IAUC 4163) from the orbital elements on MPC 10377: 1986 ET R.A. (1950.0) Decl. p r m1 Mar. 11 5 32.34 +36 49.7 1.776 2.103 14.5 21 5 52.36 +36 35.5 31 6 12.89 +36 12.4 2.089 2.209 15.0 Apr. 10 6 33.65 +35 40.2 20 6 54.43 +34 59.4 2.411 2.319 15.6 30 7 15.03 +34 10.4 May 10 7 35.32 +33 13.8 2.732 2.432 16.0 20 7 55.21 +32 10.3 30 8 14.61 +31 00.8 3.043 2.547 16.5 SUPERNOVA 1986A IN NGC 3367 W. S. Penhallow, Physics Department, University of Rhode Island, also reports a precise position for this object (cf. IAUC 4179): R.A. = 10h43m57.56s, Decl. = +14deg00'50"4 (equinox 1950.0). 1986 March 20 (4195) Daniel W. E. Green
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