Spectral variability of IL cephei

The results of six years of spectroscopic studies of the Herbig Be star IL Cep (HD216629) are reported. Various spectral parameters of the H α and H β emission lines and those of the He I λ 5876 Å absorption feature are found for the first time to have exhibited slow variations in 2006–2011 and to h...

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Veröffentlicht in:Astrophysical bulletin 2013-04, Vol.68 (2), p.196-207
Hauptverfasser: Ismailov, N. Z., Bakhaddinova, G. G., Khalilov, O. B., Mikailov, Kh. M.
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creator Ismailov, N. Z.
Bakhaddinova, G. G.
Khalilov, O. B.
Mikailov, Kh. M.
description The results of six years of spectroscopic studies of the Herbig Be star IL Cep (HD216629) are reported. Various spectral parameters of the H α and H β emission lines and those of the He I λ 5876 Å absorption feature are found for the first time to have exhibited slow variations in 2006–2011 and to have reached their extrema in 2009–2010. The Na I D1 and D2 lines reproduce, in a weaker form, the H α radialvelocity variations. It is suggested that the variations found in the spectrum of the star may be due to the presence of additional bodies in the system.
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subjects Astronomy
Astrophysics
Astrophysics and Cosmology
Emission spectroscopy
Physics
Physics and Astronomy
Spectra
Spectral emissivity
Spectral lines
Spectroscopic analysis
Spectroscopy
Spectrum analysis
Star & galaxy formation
Stars
Stars & galaxies
title Spectral variability of IL cephei
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