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Microvariability of line profiles in the spectra of OB stars : III. the supergiant ρ LEO. / Kholtygin, A. F.; Fabrika, S. N.; Burlakova, T. E.; Valyavin, G. G.; Chuntonov, G. A.; Kudryavtsev, D. O.; Kang, D.; Yushkin, M. V.; Galazutdinov, G. A.

в: Astronomy Reports, Том 51, № 11, 1005, 11.2007, стр. 920-931.

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

Harvard

Kholtygin, AF, Fabrika, SN, Burlakova, TE, Valyavin, GG, Chuntonov, GA, Kudryavtsev, DO, Kang, D, Yushkin, MV & Galazutdinov, GA 2007, 'Microvariability of line profiles in the spectra of OB stars: III. the supergiant ρ LEO', Astronomy Reports, Том. 51, № 11, 1005, стр. 920-931. https://doi.org/10.1134/S1063772907110054

APA

Kholtygin, A. F., Fabrika, S. N., Burlakova, T. E., Valyavin, G. G., Chuntonov, G. A., Kudryavtsev, D. O., Kang, D., Yushkin, M. V., & Galazutdinov, G. A. (2007). Microvariability of line profiles in the spectra of OB stars: III. the supergiant ρ LEO. Astronomy Reports, 51(11), 920-931. [1005]. https://doi.org/10.1134/S1063772907110054

Vancouver

Kholtygin AF, Fabrika SN, Burlakova TE, Valyavin GG, Chuntonov GA, Kudryavtsev DO и пр. Microvariability of line profiles in the spectra of OB stars: III. the supergiant ρ LEO. Astronomy Reports. 2007 Нояб.;51(11):920-931. 1005. https://doi.org/10.1134/S1063772907110054

Author

Kholtygin, A. F. ; Fabrika, S. N. ; Burlakova, T. E. ; Valyavin, G. G. ; Chuntonov, G. A. ; Kudryavtsev, D. O. ; Kang, D. ; Yushkin, M. V. ; Galazutdinov, G. A. / Microvariability of line profiles in the spectra of OB stars : III. the supergiant ρ LEO. в: Astronomy Reports. 2007 ; Том 51, № 11. стр. 920-931.

BibTeX

@article{aefacec5945044ef80adfd514f1f7713,
title = "Microvariability of line profiles in the spectra of OB stars: III. the supergiant ρ LEO",
abstract = "We observed the bright supergiant ρ Leo (B1 lab) in January-February 2004 using the 6-m telescope of the Special Astrophysical Observatory (Russia) and the 1.8-m telescope of the Bohyunsan Optical Astronomy Observatory (South Korea). 47 spectra with high time resolution (4-10 min), signal-to-noise ratios 300-1000, and spectral resolutions 45 000-60 000 were obtained. We detected variability in the HeI, SiII, SiIII, and NII line profiles, which may be due to rotational modulation of the profiles and photospheric pulsations of ρ Leo. The possible influence of the stellar magnetic field on the line-profile variations is discussed.",
keywords = "B-TYPE STARS, MAGNETIC-FIELD, TIME-SERIES, H-ALPHA, WIND CONFINEMENT, VARIABILITY, SPECTROSCOPY, PULSATIONS, ORIONIS, SEARCH",
author = "Kholtygin, {A. F.} and Fabrika, {S. N.} and Burlakova, {T. E.} and Valyavin, {G. G.} and Chuntonov, {G. A.} and Kudryavtsev, {D. O.} and D. Kang and Yushkin, {M. V.} and Galazutdinov, {G. A.}",
note = "Funding Information: ACKNOWLEDGMENTS This work was supported by the Russian Foundation for Basic Research (project no. 05-02-16995a), the Program of Support of Leading Scientific Schools of the Russian Federation (grant no. NSh-8542.2006.2), and a Presidential Grant of the Russian Federation for the Support of Young Russian PhDs in Science (grant no. MK-874.2004.2). G.G.V. is grateful to the Ministry of Science and Technology of South Korea (Korea MOST), which supported him with grant M1-0222-00-0005, and the South Korean Science and Technology Society (KOFST) for financial support in the framework of KASI (the Brain Pool Program).",
year = "2007",
month = nov,
doi = "10.1134/S1063772907110054",
language = "English",
volume = "51",
pages = "920--931",
journal = "Astronomy Reports",
issn = "1063-7729",
publisher = "МАИК {"}Наука/Интерпериодика{"}",
number = "11",

}

RIS

TY - JOUR

T1 - Microvariability of line profiles in the spectra of OB stars

T2 - III. the supergiant ρ LEO

AU - Kholtygin, A. F.

AU - Fabrika, S. N.

AU - Burlakova, T. E.

AU - Valyavin, G. G.

AU - Chuntonov, G. A.

AU - Kudryavtsev, D. O.

AU - Kang, D.

AU - Yushkin, M. V.

AU - Galazutdinov, G. A.

N1 - Funding Information: ACKNOWLEDGMENTS This work was supported by the Russian Foundation for Basic Research (project no. 05-02-16995a), the Program of Support of Leading Scientific Schools of the Russian Federation (grant no. NSh-8542.2006.2), and a Presidential Grant of the Russian Federation for the Support of Young Russian PhDs in Science (grant no. MK-874.2004.2). G.G.V. is grateful to the Ministry of Science and Technology of South Korea (Korea MOST), which supported him with grant M1-0222-00-0005, and the South Korean Science and Technology Society (KOFST) for financial support in the framework of KASI (the Brain Pool Program).

PY - 2007/11

Y1 - 2007/11

N2 - We observed the bright supergiant ρ Leo (B1 lab) in January-February 2004 using the 6-m telescope of the Special Astrophysical Observatory (Russia) and the 1.8-m telescope of the Bohyunsan Optical Astronomy Observatory (South Korea). 47 spectra with high time resolution (4-10 min), signal-to-noise ratios 300-1000, and spectral resolutions 45 000-60 000 were obtained. We detected variability in the HeI, SiII, SiIII, and NII line profiles, which may be due to rotational modulation of the profiles and photospheric pulsations of ρ Leo. The possible influence of the stellar magnetic field on the line-profile variations is discussed.

AB - We observed the bright supergiant ρ Leo (B1 lab) in January-February 2004 using the 6-m telescope of the Special Astrophysical Observatory (Russia) and the 1.8-m telescope of the Bohyunsan Optical Astronomy Observatory (South Korea). 47 spectra with high time resolution (4-10 min), signal-to-noise ratios 300-1000, and spectral resolutions 45 000-60 000 were obtained. We detected variability in the HeI, SiII, SiIII, and NII line profiles, which may be due to rotational modulation of the profiles and photospheric pulsations of ρ Leo. The possible influence of the stellar magnetic field on the line-profile variations is discussed.

KW - B-TYPE STARS

KW - MAGNETIC-FIELD

KW - TIME-SERIES

KW - H-ALPHA

KW - WIND CONFINEMENT

KW - VARIABILITY

KW - SPECTROSCOPY

KW - PULSATIONS

KW - ORIONIS

KW - SEARCH

UR - http://www.scopus.com/inward/record.url?scp=36649031249&partnerID=8YFLogxK

U2 - 10.1134/S1063772907110054

DO - 10.1134/S1063772907110054

M3 - Article

VL - 51

SP - 920

EP - 931

JO - Astronomy Reports

JF - Astronomy Reports

SN - 1063-7729

IS - 11

M1 - 1005

ER -

ID: 9369790