A spectroscopic study of Nova Oph 1994

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

Feb 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997cha%26a..21..313h&link_type=abstract

Chinese Astronomy and Astrophysics, Volume 21, Issue 3, p. 313-318.

Astronomy and Astrophysics

Astrophysics

Scientific paper

We 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 FeII emission lines in the early spectra indicate that it belongs to FeII 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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