MM Hya likely superoutburst Rod Stubbings reports the SU UMa-type dwarf nova MM Hya (PG 0911-066) is undergoing a bright outburst (likely superoutburst). The latest reported outburst (superoutburst) occurred in 1998 March (J. Kemp, vsnet-alert 1524), when the presence of superhumps was first revealed (R. Novak, vsnet-alert 1529). The best determined superhump period is P=0.05862 +/- 0.00011 d (Harvey and Vanmunster, CVC 163, also vsnet-alert 1532). YYMMDD(UT) mag observer 990406.407 <148 (R. Stubbings) 990408.397 134 (R. Stubbings) More information in vsnet-alert 1525: http://vsnet.kusastro.kyoto-u.ac.jp/vsnet/Mail/vsnet-alert/msg01525.html Time-resolved photometry of the present likely superoutburst are equally encouarged. Regards, Taichi Kato