Re: More on IM Nor Yamaoka-san wrote: > Actually, on DSS2 I or R image, this "star" is composed of at least > three stars, line-uping ENE-WSW. Liller's position is moderately > coinsident with the most eastern star, whose rough position end > figures are: 26s.42, 17".9. This possible identification seems to support a minimal outburst amplitude of 11.5 mag (Wyckoff and Wehinger (1979) PASP 91, 173). This value is quite unexpected for a slow recurrent nova! (as well as strong [O I] line, suggesting a fair amount of ejecta comparable to those of classical novae). Similar (but with a lesser degree) of surprise has been found in CI Aql. It may be possible we are encountering a new era of discoveries of a new class of recurrent novae! The faint quiescent counterpart could also be explained if the system was seen near edge-on. In such a case, we can expect that eclipse can emerge (as in U Sco and CI Aql) as the nova fades. Continuous photometry would be helpful in testing this possibility! Regards, Taichi Kato