Electronic Telegram No. 2617 Central Bureau for Astronomical Telegrams INTERNATIONAL ASTRONOMICAL UNION CBAT Director: Daniel W. E. Green; Hoffman Lab 209; Harvard University; 20 Oxford St.; Cambridge, MA 02138; U.S.A. e-mail: cbatiau@eps.harvard.edu (alternate cbat@iau.org) URL http://www.cbat.eps.harvard.edu/index.html Prepared using the Tamkin Foundation Computer Network NEW VARIABLE STAR IN PISCES U. Munari, Istituto Nazionale di Astrofisica, Padova Astronomical Observatory; and P. Valisa, M. Marinelli, and S. Dallaporta, "Asiago Novae and Symbiotic Stars" (ANS) collaboration, have observed the new variable star announced on CBET 2616. CCD photometry provides V = 13.83, B-V = +0.01, V-Ic = +0.11 for Jan. 1.71 UT. Absolute optical spectrophotometry (range 400-710 nm; dispersion 0.21 nm/pixel) was obtained with the 0.60-m telescope of the Schiaparelli Observatory in Varese on Jan. 1.74 UT. The spectrum is dominated by a featureless hot continuum with no line visible in emission, and H_beta, H_gamma, and H_delta in absorption with equivalent widths of 0.77, 0.52, and 0.38 nm, respectively. No obvious line is visible at the H_alpha wavelength, suggesting that an emission core could be filling in the expected absorption line. The Balmer lines are wide (the FWHM of H_beta is 4.3 nm) and are red- shifted by +120 km/s, excluding that the variable could be a classical nova observed close to maximum light. The object has the appearance expected from a cataclysmic variable in outburst. B. Skiff, Lowell Observatory, notes that this object shows up also in the Sloan DR7 catalogue as an ultraviolet-bright object (Sloan mag about 21 in all five passbands on 2005 Sept. 13 UT), at the following position: R.A. = 23h04m25s.88, Decl. = +6d25'45".7 (equinox 2000.0; formal uncertainty 0".11). NOTE: These 'Central Bureau Electronic Telegrams' are sometimes superseded by text appearing later in the printed IAU Circulars. (C) Copyright 2011 CBAT 2011 January 2 (CBET 2617) Daniel W. E. Green