Hα profile variabilities in the spectrum of the star WW Vul in 2006–2010

We present the results of our studies of the H α line in the spectrum of a UX Ori star (WW Vul) based on our spectroscopic observations performed with the 2-m telescope at the Shamakhi Astrophysical Observatory, the National Academy of Sciences of Azerbaijan, in 2006–2010. We have detected variabili...

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Veröffentlicht in:	Astronomy letters 2014-06, Vol.40 (6), p.343-352
Hauptverfasser:	Medzhidova, S. O., Mikailov, Kh. M., Rustamov, B. N.
Format:	Artikel
Sprache:	eng
Schlagworte:	Astronomy Astrophysics and Astroparticles Observations and Techniques Physics Physics and Astronomy
Online-Zugang:	Volltext
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