SIMBAD references

A. Pigulski, Astronomical Institute, Wroclaw University, writes that he obtained a single spectrogram of the variable with the 1.9-m Radcliffe telescope (+ GIRAFFE echelle spectrograph; range 425-680 nm; resolution 32000) of the South African Astronomical Observatory on May 13.89 UT. The star shows very strong and broad emission in H-alpha, H-beta, and H-gamma. The peak flux of the H-alpha emission is roughly ten times stronger than that of the continuum. The FWHM of the Balmer lines (as measured from H-alpha and H-beta) corresponds to the velocity of 2300 km/s. In addition, the Fe II emission features at 490-540 nm, characteristic for a nova at an early stage of evolution, can be clearly seen in the spectrum.