Spectroscopic Variability of Supergiant Star HD14134, B3Ia

Profile variations in the H α and H β lines in the spectra of the star HD14134 are investigated using observations carried out in 2013–2014 and 2016 with the 2-m telescope at the Shamakhy Astrophysical Observatory. The absorption and emission components of the H α line are found to disappear on some...

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Veröffentlicht in:	Journal of astrophysics and astronomy 2017-06, Vol.38 (2), p.1, Article 20
1. Verfasser:	Maharramov, Y. M.
Format:	Artikel
Sprache:	eng
Schlagworte:	Absorption Astronomy Astrophysical observatories Astrophysics and Astroparticles Atmosphere Displacement Emission spectroscopy Giant stars Line spectra Observations and Techniques Physics Physics and Astronomy Spectrograms Spectrum analysis Stellar winds Wavelengths
Online-Zugang:	Volltext
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