Electronic Telegram No. 1029 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 VULPECULAE 2007 U. Munari, Istituto Nazionale di Astrofisica, Padova Astronomical Observatory; and S. Moretti and S. Tomaselli, ANS (Asiago Novae and Symbiotic stars) collaboration, write that a low-resolution (400-780 nm, 0.54 nm/pixel) spectrum of N Vul 2007 (cf. IAUC 8861, 8862) was obtained on Aug. 9.945 UT with a 0.42-m reflector in Bastia (Ravenna), Italy, showing a blue continuum with strong hydrogen Balmer and Fe II multiplet-42 emission lines, all displaying deep P-Cyg profiles, with absorption components displaced on average by -2100 km/s from emission components. Fe II multiplets 38, 48, 49, and 74, and O I 777.2-nm, are seen in absorption, with weak emission components. He I 587.6-, 667.8-, and 706.5-nm are seen in weak absorption. The object is therefore confirmed as a nova, of the Fe II type, observed close to maximum optical brightness. CCD photometry on Aug. 9.889 yields V = 8.24 and B-V = +0.52. CCD magnitudes reported to the Central Bureau for N Vul 2007: Aug. 5.518 UT, [13.0 (Y. Nakamura, Kameyama, Mie, Japan, 135-mm f/2.8 telephoto lens; communicated via H. Yamaoka, Kyushu University); Aug. 9.146, V = 8.42 +/- 0.01 (W. G. Dillon, Missouri City, TX, U.S.A., remotely using a robotic telescope near Mayhill, NM); Aug. 9.33, V = 8.30, B-V = +0.45; V-R = +0.40 (E. Guido and G. Sostero, observing remotely with a telescope near Mayhill, NM, U.S.A.); Aug. 9.512, 8.4 (H. Abe, Yatsuka-cho, Matsue, Shimane-ken, Japan; via S. Nakano, Sumoto, Japan). Visual magnitude estimate: Aug. 9.862, 8.6 (C. Labordena, Castello, Spain). NOTE: These 'Central Bureau Electronic Telegrams' are sometimes superseded by text appearing later in the printed IAU Circulars. (C) Copyright 2007 CBAT 2007 August 10 (CBET 1029) Daniel W. E. Green