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Abstrakty
Profile variations in the Hα and Hβ lines in the spectra of the star HD 225094 are investigated using observations carried out in 2013-2014 with the 2-m telescope at the Shamakhy Astrophysical Observatory. The spectral resolution of the collected spectra is approximately 15 000. The absorption and emission components of the Hα line are found to disappear on some observational epochs. It is suggested that the observational evidence for the non-stationary atmosphere of HD 225094 can be associated in part with non-spherical stellar wind.
Słowa kluczowe
Czasopismo
Rocznik
Tom
Strony
205--214
Opis fizyczny
Bibliogr. 17 poz., tab., wykr.
Twórcy
autor
- Shamakhy Astrophysical Observatory, Azerbaijan National Academy of Sciences, Yu. Mammadaliyev settlement, Shamakhy district, Republic of Azerbaijan
Bibliografia
- Galazutdinov, G.A. 1992, Preprint SAO RAN, Spets. Astrofiz. Observ., Nizhnii Arkhyz, KChR, 92.
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- Maharramov, Y.M. 2013a, Astronomy Reports, 57, 303.
- Maharramov, Y.M. 2013b, Kinematics and Physics of Celestial Bodies, 29, 2.78
- McErlean, N.D., Lennon, D.J., and Dufton, P.L. 1999, A&A, 349, 553.
- Mikailov, Kh.M., Khalilov, V.M., and Alekberov, I.A. 2005, Tsirk. Shamakhy Astrophys. Observ., 109, 21.
- Pasok, A., and Kolka, I. 1992, IBVS, 3804.
- Prinja, R.K., and Massa, D.L. 2010, A&A, 521, 55.
- Rimoldini, L., et al. 2012, MNRAS, 427, 2917.
- Rosendhal, J.D. 1973, ApJ, 186, 909.
- Sobolev, V.V. 1947, in: “Moving Envelopes of Stars”, Leningrad.
- Sobolev, V.V. 1985, in: “Course in Theoretical Astrophysics”, Moscow, Izdatel’stvo Nauka.
Typ dokumentu
Bibliografia
Identyfikator YADDA
bwmeta1.element.baztech-e382cc9f-26b7-44f9-ae2b-478942fe2f3d