Re: [vsnet-chat 2874] CI Aql > Concerning the (recurrent) nova in Aquila, shouldn't it be fading by now. > As stated in the IAU Circular No. 7409 :'The spectrum is similar to those of > fast novae a few weeks after maximum.' Please have a look at the spectrum on the VSNET CI Aql page. At least this is not a spectrum of a nova at maximum. The expansion velocity inferred from the FWHM looks smaller than those of very fast novae like U Sco etc., so the object may be somewhere intermediate between U Sco-type fast recurrent novae and T Pyx. Regards, Taichi Kato