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Circular No. 8253 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) V838 MONOCEROTIS M. Mikolajewski and T. Tomov, Uniwersytet Mikolaja Kopernika; R. Kurtev, Sofia University; L. Georgiev, Universidad Nacional Autonoma de Mexico; and A. Wolszczan, Pennsylvania State University, write that they obtained UBVI and H_alpha images of V838 Mon and its light echo with the 1.5-m telescope at San Pedro Martir on Oct. 18.5 UT, noting that V838 Mon recently has become bluer (cf. IAUC 8202, 8210) and comparable in bands U and B to its previously reported B3-V companion (IAUC 8005). V838 Mon itself, and an additional star about 1" to the southeast, are clearly visible in their U images. The B-band centroid of the V838 Mon image is shifted in the same direction, while frames at longer wavelengths display only one star at this position. The authors' low-resolution spectral observations of V838 Mon obtained on Jan. 27.2 and Mar. 24.1 with the 10-m Hobby-Eberly Telescope (range 430-730 nm, resolving power 650) also show a composite spectrum. The blue and yellow regions are dominated by a reddened (V about 15.9; B about 16.5), normal B3-V star. The red part of the spectrum is characterized by strong features belonging to an extremely cool (L-type?) supergiant, evidently a remnant of the V838 Mon outburst. The analyses of the interstellar features and reddening suggest that the B3-V star is a blending objects lying about 1000 pc behind V838 Mon. Two rings are apparent in the current light echo visible on the new V, I, and H_alpha images: an almost concentric outer circle with radius about 50" and an eccentric inner ellipse with half-axes of about 25" x 32". COMET 158P/KOWAL-LINEAR Following the reported identification on IAUC 8247 of P/2001 RG_100 (LINEAR) with C/1979 O1 (Kowal), the IAU Committee on Small- Body Nomenclature has agreed to rename this comet 158P/Kowal-LINEAR. NOVAE IN M31 Further to IAUC 8238, M. Fiaschi, D. Tiveron, and L. Milani report the discovery of an apparent nova located at R.A. = 0h43m00s.75, Decl. = +41o11'26".7 (equinox 2000.0), which is 185" east and 282" east of the center of M31. Available H_alpha magnitudes: Nov. 29, [18; Dec. 3.722 UT, 16.6; 5.776, 15.8. They also report H_alpha magnitudes of the new apparent nova reported on IAUC 8248: Nov. 4.966, 17.2; 29.760, 17.0; Dec. 3.722, 17.3; 5.776, 18:. (C) Copyright 2003 CBAT 2003 December 8 (8253) Daniel W. E. Green
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