[vsnet-outburst 11045] (fwd) Re: V407 Cyg outburst spectra

[Taichi Kato]

The V3890 Sgr and V745 Sco spectra in the low resolution UV at this
stage showed two components, one from the shock expansion of the ejecta
in the red giant wind and the other from the expanding ionization
front.  This should develop in time if the eruptions are similar (see
the RS Oph 2006 conference, ASP Conf series, ed. Evans and Bode).

steve shore