SIMBAD references

S. Siviero, P. M. Marrese, and U. Munari, Asiago Observatory, write that the spectroscopic evolution of the possible nova reported on IAUC 8190 and 8191, as monitored with the Asiago 1.22-m and 1.82-m telescopes, allows them to classify the object as a normal nova. Spectra (with AFOSC in echelle mode; range 360-860 nm; resolving power 3800) obtained on Sept. 6.83 UT display a well- developed emission-line spectrum dominated by Fe II lines (multiplets 27, 28, 37, 38, 40, 42, 48, 49, 73, and 74, among others), and Balmer lines characterized by a rapid decrement. Most lines display complex P-Cyg profiles, those of the Na I D lines having an emission width of 900 km/s and a terminal velocity of 1150 km/s for the absorption, with superimposed marked interstellar components. No nebular lines have so far developed.