Circular No. 4551 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 T PYXIDIS E. Schweitzer, AFOEV, Strasbourg, reports that M. Verdenet, Bourbon-Lancy, France, has observed a rise in brightness of this recurrent nova to mv = 12.8 on Feb. 21.93 UT. PKS 0823-22 E. G. Tanzi, CNR, Milan; P. Bouchet, European Southern Observatory, La Silla; R. Falomo, Padua; and L. Maraschi and A. Treves, University of Milan, telex: "The BL-Lac object PKS 0823-22 was observed at optical (ESO 1.52-m telescope + CCD spectrograph) and infrared (ESO 2.2-m telescope + InSb photometer) frequencies on Jan. 7.4 and 8.4 UT, and found to be in its brightest state ever recorded: V = 15.7, K = 12.0. An absorption doublet was apparent at 534.0 and 535.4 (+/- 0.1) nm, with equivalent widths 0.23 and 0.12 nm. Identification with Mg II (279.6, 280.3 nm) yields z >/= 0.910. For A(V) = 0.6 (as derived from H I columnar density), M(abs) </= -29.1, placing the object among the most luminous of its class (cf. Veron-Cetty and Veron 1987, ESO Scientific Report No. 5)." KR AURIGAE R. Monella, Covo, Italy, notes that this object has brightened rapidly, as indicated by the following visual magnitude estimates: Feb. 13.910 UT, 15.0; 15.886, 15.0; 16.899, 14.9; 19.890, 13.7; 20.910, 13.6. E. Waagen, AAVSO, remarks that no known similar rapid increase in brightness has occurred since at least 1983. COMET LILLER (1988a) Total visual magnitude estimates (L = reflector): Feb. 7.09 UT, 8.6 (R. Keen, Mt. Thorodin, CO, 0.32-m L); 9.75, 8.5 (A. Boattini, Florence, Italy, 0.33-m L); 13.13, 8.3 (C. S. Morris, Whitaker Peak, CA, 20x80 binoculars); 15.08, 8.0 (Keen, 0.15-m L); 22.01, 8.3 (G. R. Chester, Rixeyville, VA, 0.14-m L). NEPTUNE II (NEREID) Corrigendum. The number 3822 +/- 700, given at the end of the item on IAUC 4542, refers not to the Neptune/Triton mass ratio, but to 1000/J2, where J2 is the effective dipole form factor due to both the oblateness of Neptune and the presence of Triton. 1988 February 22 (4551) Daniel W. E. Green
Our Web policy. Index to the CBAT/MPC/ICQ pages.