Electronic Telegram No. 2139 Central Bureau for Astronomical Telegrams INTERNATIONAL ASTRONOMICAL UNION M.S. 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://www.cfa.harvard.edu/iau/cbat.html NOVA OPHIUCHI 2010 Hiroyuki Maehara, Kwasan Observatory, Kyoto University, reports that a low-resolution spectrum (range 400-800 nm) of this object (cf. CBET 2128) was obtained on Jan. 22.890 UT with the 25-cm telescope at the Kwasan Observatory. The spectrum shows H_alpha and Fe II emission lines and suggests that this object is a classical nova just after maximum. Maehara also writes that CCD images of the nova obtained with a 25-cm telescope at the Kwasan Observatory yield the following magnitudes: Jan. 16.875, I_c = 7.92; 16.875, R_c = 8.37; 16.876, V = 8.77; 16.877, B = 9.54. Further to CBET 2128, S. Nakano reports that H. Nishimura measured mag 8.0 for the nova on Jan. 16.86 UT. Nakano adds that K. Kadota subsequently measured a star on a U.K. Schmidt Telescope plate (via the Digitized Sky Survey) taken on 1997 Mar. 31 to have red mag 16.7 and to be located at R.A. = 17h39m40s.96, Decl. = -21d39'45".4 (equinox 2000.0). W. Vollmann, Vienna, Austria, reports the following green-filtered CCD magnitudes (approximately visual) measured from images taken by Hermann Koberger (Vilaflor, Tenerife, Spain): Jan. 18.299 UT, 8.4; 20.289, 9.0; 21.273, 9.3; 22.250, 9.5. U. Munari, Istituto Nazionale di Astrofisica, Padova Astronomical Observatory; and S. Dallaporta, Asiago Novae and Symbiotic Stars (ANS) collaboration, report photometry for this nova: Jan. 19.23 UT, V = 9.24, B-V = +0.85; 20.23, V = 9.15, B-V = +0.86; 22.22, V = 9.51, B-V = +0.74. NOTE: These 'Central Bureau Electronic Telegrams' are sometimes superseded by text appearing later in the printed IAU Circulars. (C) Copyright 2010 CBAT 2010 January 22 (CBET 2139) Daniel W. E. Green