Nova Sgr 2001 progenitor If the 16-17th mag, red star close to the outbursting object is confirmed as the progenitor of the nova, the nova may be a recurrent nova, having a bright quiescent counterpart and a high ejection velocity. In such a case, the evolution of the nova may be extremely rapid. Dense follow-up observations (including nightly spectroscopy, multicolor photometry etc.) are very crucial. A search for past outburst may be meaningful. Regards, Taichi Kato