HD 16523 and HD 17638 - Possible Wolf-Rayet WO-type stars

Astronomy and Astrophysics – Astrophysics

Scientific paper

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Emission Spectra, Spectrum Analysis, Stellar Spectrophotometry, Visible Spectrum, Wolf-Rayet Stars

Scientific paper

Spectrograms (dispersion = 5 A/mm) obtained with the 2-m telescope of the Shemakha Astrophysical Observatory (Azerbaidzhan) were used to determine the spectral subtypes of the WR-type stars HD 16523 and HD 17638. Since these stars have optical spectra containing the emission doublet OVI 3811, 3834 A, they may be related to the WO5 subtype. Classification criteria for the WO5 subtype are presented.

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