Dear SN watchers, A bright southern supernova has been discovered by Chile astronomer. IAUC 7061 reports that SN 1998ew was discovered on Nov. 23.02 UT, when its magnitude was B about 14. It has been revealed that it is of type II supernovae in early phase (near maximum) by ESO spectroscopy. The position of this new star is R.A. = 20h44m32s.1, Decl. = -68o43'37" (2000.0), which is about 5" west and 73" north from the spiral host galaxy. It is well outside of the visible disk, and between two foreground (about 15 mag) USNO stars. Current reports about magnitudes are (all of them are from IAUC): Nov. 11.06 >195B Cerro El Roble Nov. 23.02 14:B Cerro El Roble Nov. 27.05 152:V ESO Nov. 27.05 149:R ESO The recession velosity of NGC 6943 is around 3000 km s-1, then the typical SN II on this galaxy is expected to be about 16 mag or so on its maximum. The reported magnitudes are well brighter than this value, so the followup magnitude estimates are surely encouraged for this peculiar SN. There has been reported some bright SNeII, such as SN 1998S. But from the information on IAUC, the spectrum of SN 1998ew does not resemble that of SN 1998S (narrow-line SN II). ESO reporters suggest that SN 1998ew shows some resemblance to SN 1979C. Sincerely Yours, Hitoshi Yamaoka, Kyushu Univ., Japan yamaoka@rc.kyushu-u.ac.jp