Electronic Telegram No. 855 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://cfa-www.harvard.edu/iau/cbat.html V1281 SCORPII = ANOTHER POSSIBLE NOVA IN SCORPIUS H. Naito and S. Narusawa, Nishi-Harima Astronomical Observatory (NHAO); and H. Yamaoka, Kyushu University, report that a low-resolution spectrogram (range 410-670 nm; resolution 1600 at H_alpha) of the possible nova reported on IAUC 8810 was obtained on Feb. 21.84 UT with the 2.0-m NAYUTA telescope (+ MALLS). The spectrum shows a broad H_alpha line with a P-Cyg profile (the FWHM of the emission component is about 1800 km/s), along with many other weaker lines, indicating that the star is indeed a classical nova. A narrow Na I D absorption feature suggests the existence of considerable interstellar reddening. N. N. Samus, Institute of Astronomy, Russian Academy of Sciences, reports that this nova has been given the designation V1281 Sco. NOTE: These 'Central Bureau Electronic Telegrams' are sometimes superseded by text appearing later in the printed IAU Circulars. (C) Copyright 2007 CBAT 2007 February 22 (CBET 855) Daniel W. E. Green