On Mon, 19 Aug 1996 tkato said to all... >Following observations reported to vsnet-obs seem to indicate Nova >Sgr 1996 is undergoing a distinct re-brightening. <snip> >Confirmation is strongly encouraged. Such large amplitude >fluctuations during the early post-maximum stage of novae were >observed markedly in V443 Sct (Nova Sct 1989), and more recently in >Nova Sgr 1994 No.2, the latter accompanied by a subsequent deep >dust minimum. Close monitoring of another variety of recent series >of "slow novae" would be interesting. Nova Circini 1995 also showed similar behaviour, starting a couple of weeks after maximum. Very interesting to watch, because you could never be sure what it would be doing next.... cheers, Fraser Farrell Variable Stars Group Astronomical Society of South Australia `[1;32;44mNet-Tamer V 1.04 - Registered