A spectroscopic study of Nova Oph 1994

We observed Nova Oph 1994 with a Zeiss universal spectrograph attached to the 2.16m 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...

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Bibliographic Details
Published inChinese astronomy and astrophysics Vol. 21; no. 3; pp. 313 - 318
Main Authors Hu, Jing-yao, Jiang, Xiao-jun
Format Journal Article
LanguageEnglish
Published Elsevier B.V 1997
Subjects
nova
Nova Oph 1994
spectra
spectra
Nova Oph 1994
nova
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Summary:We observed Nova Oph 1994 with a Zeiss universal spectrograph attached to the 2.16m 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.
ISSN:0275-1062
1879-128X
DOI:10.1016/S0275-1062(97)00041-6