[IAUC] CBET 2617: 20110102 : NEW VARIABLE STAR IN PISCES

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                                                  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 en eps.harvard.edu (alternate cbat en 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      superseded by text appearing later in the printed IAU Circulars.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



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