MM Sco outburst, recent data The SU UMa-type dwarf nova MM Sco is undergoing an outburst. The superhump period of MM Sco (0.06136 d) indicates that the object belongs to the short-period SU UMa-type group. Although the current brightness is not comparably bright to past superoutbursts, the object would be a potential time-series observation target. Web information: http://vsnet.kusastro.kyoto-u.ac.jp/vsnet/DNe/mmsco.html YYYYMMDD(UT) mag observer 20030424.574 <140 (Rod Stubbings) 20030425.625 <140 (Rod Stubbings) 20030426.610 <144 (Rod Stubbings) 20030427.462 <148 (Rod Stubbings) 20030428.572 <144 (Rod Stubbings) 20030504.528 <144 (Rod Stubbings) 20030505.594 <144 (Rod Stubbings) 20030509.619 <144 (Rod Stubbings) 20030510.660 <144 (Rod Stubbings) 20030512.739 <144 (Rod Stubbings) 20030524.540 <140 (Rod Stubbings) 20030526.422 140 (Rod Stubbings) 20030526.576 139 (Rod Stubbings) Regards, Taichi Kato VSNET Collaboration team
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