Dear vsneters, Photometry by William (Bill) Liller of Nova Mus 98 during ~4 hr in 27/1/99 through a 'broad' V filter (8-inch telescope) reveals a possible photometric period of ~2.5 hr. The full peak amplitude is about 0.15 mag. More observations are required in order to confirm this periodicity. The nova is most probably in the transition phase. The physical mechanism that causes these oscillations is still unknown. Among the possibilities, there was a suggestion that these are oscillations of the common envelope. A different suggestion is that they instabilities in the accretion disc (similar to dwarf nova outbursts). If the period is confirmed, it means that we see into the binary system, so the common envelope explanation might be ruled out. In addition, if the white dwarf doesn't posses a strong magnetic field, such a short period (which is probably the orbital period) should be accompanied by a second superhump period, a few per longer than the orbital period. Any continuous run for more than ~2.5 hr in any filter (I is probably preferred, clear is o.k., too) should be very useful. I enclose below the data. Enjoy! Regards, Alon Retter Keele University =================== JD dV (-2451205) .6116 .65 .6131 .76 .6165 .77 .6199 .81 .6234 .65 .6268 .70 .6302 .78 .6337 .66 .6371 .68 .6405 .62 .6440 .67 .6474 .69 .6508 .62 .6543 .61 .6577 .68 .6611 .74 .6646 .50 .6680 .67 .6714 .74 .6749 .67 .6783 .69 .6817 .68 .6852 .73 .6886 .70 .6920 .73 .6955 .70 .6989 .74 .7023 .76 .7058 .75 .7092 .72 .7126 .78 .7161 .66 .7195 .83 .7229 .72 .7263 .69 .7298 .73 .7332 .71 .7367 .68 .7401 .71 .7435 .68 .7470 .65 .7504 .70 .7538 .66 .7573 .71 .7607 .66 .7641 .65 .7676 .72