Investigation of the Hα spectral line and the Na D sodium doublet in the spectrum of the post-AGB star HD 161796
Variability of the profile of the H α line and the Na D sodium doublet in the spectrum of HD 161796 was studied based on the spectrograms obtained with the 2-meter telescope of Shamakhy Astrophysical Observatory (National Academy of Sciences of Azerbaijan). It was found that the radial velocity and...
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Veröffentlicht in: | Kinematics and physics of celestial bodies 2014-11, Vol.30 (6), p.288-295 |
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