BELGIAN ASTRONOMICAL SOCIETY V.V.S. - Working Group Variable Stars Cataclysmic Variables Circular No.44 1995, June 25 Ed.: T. Vanmunster, Walhostraat 1A, 3401 Landen, BELGIUM Internet: tvanmuns@innet.be TEL. 32-11-831504 P. Van Cauteren, de Borrekenslaan 54, 2630 Aartselaar, BELGIUM Internet: pvancaut@innet.be TEL. 32-3-8774098 =================================================================== V1113 Cyg [UGSU, 14p - <17p] ============================ This dwarf nova, which is part of the Recurrent Objects Programme (TA/BAAVSS), is reported in outburst by Tonny Vanmunster, Landen, Belgium. Eric Broens, Mol, Belgium has confirmed the outburst. 1995 06 21.913 UT, [14.2 (T. Vanmunster, 0.35-m refl., seq: VSOLJ); 06 24.965 UT, 13.9 (T. Vanmunster); 06 24.972 UT, 13.9 (E. Broens, 0.35-m refl., seq: VSOLJ); During the September 1994 outburst of V1113 Cyg, Taichi Kato (Ouda Station, Kyoto University, Japan) made V-band CCD photometry observations, that clearly revealed the presense of superhumps in the light curve. The super- humps had an amplitude of 0.23 mag (V) and a period a bit shorter than 2 hours (CVC 15). Apart from this professional observation, we could trace no further information on V1113 Cyg. V1113 Cyg was last seen in outburst on April 19, 1995 by Gary Poyner, UK, when it reached a max. mag. of 13.4 (CVC 35). That outburst lasted approx. 10 days, and is detailed in CVC 36. ERRATA IN CVC 43 ================ Jochen Pietz, Germany has communicated us following information with respect to his IP Peg observation, listed in CVC 43 : "The day given in my original observation report was wrong, and the correct time should be 1995 June 20.029 UT instead of 19.029 UT. Hence, my observation was no independent discovery. I used a 40-cm reflector." Tonny Vanmunster