A spectroscopic study of Nova Oph 1994.

Details A spectroscopic study of Nova Oph 1994. A spectroscopic study of Nova Oph 1994.

Apr 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997acaps..17..175h&link_type=abstract

Acta Astrophys. Sin., Vol. 17, No. 2, p. 175 - 181

Astronomy and Astrophysics

Astrophysics

Novae: Spectra, Novae: Iron Lines

Scientific paper

The authors observed Nova Oph 1994 with a Zeiss universal spectrograph attached to the 2.16 m reflector at the Xinglong Station, Beijing Astronomical Observatory. The strong Fe II emission lines in the early spectra indicate that it belongs to Fe II novae, but the multi-peaked structure of the emission lines is rather rare for this subtype. The spectral characteristics and their evolution are discussed.

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