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Microvariability of line profiles in the spectrum of the star ι Her. / Kholtygin, A. F.; Galazutdinov, G. A.; Burlakova, T. E.; Valyavin, G. G.; Fabrika, S. N.; Lee, B. C.

в: Astronomy Reports, Том 50, № 3, 01.03.2006, стр. 220-231.

Результаты исследований: Научные публикации в периодических изданиях › статья › Рецензирование

Harvard

Kholtygin, AF, Galazutdinov, GA, Burlakova, TE, Valyavin, GG, Fabrika, SN & Lee, BC 2006, 'Microvariability of line profiles in the spectrum of the star ι Her', Astronomy Reports, Том. 50, № 3, стр. 220-231. https://doi.org/10.1134/S1063772906030061

APA

Kholtygin, A. F., Galazutdinov, G. A., Burlakova, T. E., Valyavin, G. G., Fabrika, S. N., & Lee, B. C. (2006). Microvariability of line profiles in the spectrum of the star ι Her. Astronomy Reports, 50(3), 220-231. https://doi.org/10.1134/S1063772906030061

Vancouver

Kholtygin AF, Galazutdinov GA, Burlakova TE, Valyavin GG, Fabrika SN, Lee BC. Microvariability of line profiles in the spectrum of the star ι Her. Astronomy Reports. 2006 Март 1;50(3):220-231. https://doi.org/10.1134/S1063772906030061

Author

Kholtygin, A. F. ; Galazutdinov, G. A. ; Burlakova, T. E. ; Valyavin, G. G. ; Fabrika, S. N. ; Lee, B. C. / Microvariability of line profiles in the spectrum of the star ι Her. в: Astronomy Reports. 2006 ; Том 50, № 3. стр. 220-231.

BibTeX

@article{3f779d7401f448e8bc87055712c84c9f,
title = "Microvariability of line profiles in the spectrum of the star ι Her",
abstract = "We present the results of a search for and analysis of line-profile variations in the spectrum of the star ι Her. The observations were acquired with the 1.8 m telescope of the Bohyunsan Optical Astronomy Observatory (Republic of Korea) in May-June 2004. We obtained 69 spectra of the star with signal-to-noise ratios ≈300 and a time resolution of 5-7 min. Profile variability was revealed for six lines of HI, HeI, and SiIII, in the central parts of the lines. The variability amplitude is ≈(1-2)% in units of the intensity of the adjacent continuum. Evidence was found for cyclic variations of the lines, with periods from ≈7h to ≈2.9d. We conclude that ι Her belongs to the group of slowly pulsating stars.",
author = "Kholtygin, {A. F.} and Galazutdinov, {G. A.} and Burlakova, {T. E.} and Valyavin, {G. G.} and Fabrika, {S. N.} and Lee, {B. C.}",
year = "2006",
month = mar,
day = "1",
doi = "10.1134/S1063772906030061",
language = "English",
volume = "50",
pages = "220--231",
journal = "Astronomy Reports",
issn = "1063-7729",
publisher = "МАИК {"}Наука/Интерпериодика{"}",
number = "3",

}

RIS

TY - JOUR

T1 - Microvariability of line profiles in the spectrum of the star ι Her

AU - Kholtygin, A. F.

AU - Galazutdinov, G. A.

AU - Burlakova, T. E.

AU - Valyavin, G. G.

AU - Fabrika, S. N.

AU - Lee, B. C.

PY - 2006/3/1

Y1 - 2006/3/1

N2 - We present the results of a search for and analysis of line-profile variations in the spectrum of the star ι Her. The observations were acquired with the 1.8 m telescope of the Bohyunsan Optical Astronomy Observatory (Republic of Korea) in May-June 2004. We obtained 69 spectra of the star with signal-to-noise ratios ≈300 and a time resolution of 5-7 min. Profile variability was revealed for six lines of HI, HeI, and SiIII, in the central parts of the lines. The variability amplitude is ≈(1-2)% in units of the intensity of the adjacent continuum. Evidence was found for cyclic variations of the lines, with periods from ≈7h to ≈2.9d. We conclude that ι Her belongs to the group of slowly pulsating stars.

AB - We present the results of a search for and analysis of line-profile variations in the spectrum of the star ι Her. The observations were acquired with the 1.8 m telescope of the Bohyunsan Optical Astronomy Observatory (Republic of Korea) in May-June 2004. We obtained 69 spectra of the star with signal-to-noise ratios ≈300 and a time resolution of 5-7 min. Profile variability was revealed for six lines of HI, HeI, and SiIII, in the central parts of the lines. The variability amplitude is ≈(1-2)% in units of the intensity of the adjacent continuum. Evidence was found for cyclic variations of the lines, with periods from ≈7h to ≈2.9d. We conclude that ι Her belongs to the group of slowly pulsating stars.

UR - http://www.scopus.com/inward/record.url?scp=33645127586&partnerID=8YFLogxK

U2 - 10.1134/S1063772906030061

DO - 10.1134/S1063772906030061

M3 - Article

AN - SCOPUS:33645127586

VL - 50

SP - 220

EP - 231

JO - Astronomy Reports

JF - Astronomy Reports

SN - 1063-7729

IS - 3

ER -

ID: 36161658