V551 Sgr rare outburst! Dear Colleagues, Andrew Pearce reports that the dwarf nova V551 Sgr is undergoing a relatively rare outburst. The last outburst was in 2000 April (mv=13.9, Rod Stubbings). The object has been claimed to be a possible WZ Sge-like object, based on its large outburst amplitude (the minimum reaching the 20th magnitude). One the occasion of the 1998 October outburst, Gordon Garradd obtained time-series photometry on two nights, but the short visibility hindered a firm conclusion on the existence of superhumps. The present outburst, if confirmed, would provide an excellent opportunity to throughly study this still poorly understood dwarf nova. The VSNET Collaboration team lists the object as one of prime targets in the morning sky. YYYYMMDD(UT) mag observer 20010425.603 <140 (R. Stubbings) 20010426.860 <150 (A. Pearce) 20010429.613 <140 (R. Stubbings) 20010429.851 <153 (A. Pearce) 20010430.581 <140 (R. Stubbings) 20010430.824 <153 (A. Pearce) 20010501.608 <140 (R. Stubbings) 20010502.856 <153 (A. Pearce) 20010503.828 <153 (A. Pearce) 20010514.515 <140 (R. Stubbings) 20010515.574 <140 (R. Stubbings) 20010522.619 <152 (A. Pearce) 20010523.821 <152 (A. Pearce) 20010525.451 <140 (R. Stubbings) 20010526.833 144 (A. Pearce) Gordon Garradd has kindly provided his CCD image of V551 Sgr taken in 1998 October. The image is available at: http://ftp.kusastro.kyoto-u.ac.jp/pub/vsnet/DNe/V551_Sgr/v551sgr.jpg http://ftp.kusastro.kyoto-u.ac.jp/pub/vsnet/DNe/V551_Sgr/v551-01.fits Regards, Taichi Kato VSNET Collaboration team