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Line Profile Variability and a Possible Magnetic Field in the Spectra of Supergiant ζ Ori Aa. / Kholtygin, A.F.; Chountonov, G.A.; Dushin, V.V.

Magnetic Stars. Proceedings of the International Conference, held in the Special Astrophysical Observatory of the Russian AS, August 27- September 1, 2010, Eds: I. I. Romanyuk and D. O. Kudryavtsev. САО РАН, 2011. стр. 355-360.

Результаты исследований: Публикации в книгах, отчётах, сборниках, трудах конференцийстатья в сборнике материалов конференциинаучная

Harvard

Kholtygin, AF, Chountonov, GA & Dushin, VV 2011, Line Profile Variability and a Possible Magnetic Field in the Spectra of Supergiant ζ Ori Aa. в Magnetic Stars. Proceedings of the International Conference, held in the Special Astrophysical Observatory of the Russian AS, August 27- September 1, 2010, Eds: I. I. Romanyuk and D. O. Kudryavtsev. САО РАН, стр. 355-360. <http://adsabs.harvard.edu/abs/2011mast.conf..355K>

APA

Kholtygin, A. F., Chountonov, G. A., & Dushin, V. V. (2011). Line Profile Variability and a Possible Magnetic Field in the Spectra of Supergiant ζ Ori Aa. в Magnetic Stars. Proceedings of the International Conference, held in the Special Astrophysical Observatory of the Russian AS, August 27- September 1, 2010, Eds: I. I. Romanyuk and D. O. Kudryavtsev (стр. 355-360). САО РАН. http://adsabs.harvard.edu/abs/2011mast.conf..355K

Vancouver

Kholtygin AF, Chountonov GA, Dushin VV. Line Profile Variability and a Possible Magnetic Field in the Spectra of Supergiant ζ Ori Aa. в Magnetic Stars. Proceedings of the International Conference, held in the Special Astrophysical Observatory of the Russian AS, August 27- September 1, 2010, Eds: I. I. Romanyuk and D. O. Kudryavtsev. САО РАН. 2011. стр. 355-360

Author

Kholtygin, A.F. ; Chountonov, G.A. ; Dushin, V.V. / Line Profile Variability and a Possible Magnetic Field in the Spectra of Supergiant ζ Ori Aa. Magnetic Stars. Proceedings of the International Conference, held in the Special Astrophysical Observatory of the Russian AS, August 27- September 1, 2010, Eds: I. I. Romanyuk and D. O. Kudryavtsev. САО РАН, 2011. стр. 355-360

BibTeX

@inproceedings{4a742c3a1bc44b2ba4d0e7681c8aa321,
title = "Line Profile Variability and a Possible Magnetic Field in the Spectra of Supergiant ζ Ori Aa",
abstract = "Results of spectropolarimetric observations of the supergiant ζ Ori are reported. The fast line profile variability (LPV) with a period of about 3 hours is found and a connection of LPV with a non-radial pulsation of the star is supposed. We did not find any evidence for a moderate stellar magnetic field as reported by Bouret et. al., 2008}.",
keywords = "magnetic fields - stars",
author = "A.F. Kholtygin and G.A. Chountonov and V.V. Dushin",
year = "2011",
language = "English",
pages = "355--360",
booktitle = "Magnetic Stars. Proceedings of the International Conference, held in the Special Astrophysical Observatory of the Russian AS, August 27- September 1, 2010, Eds: I. I. Romanyuk and D. O. Kudryavtsev",
publisher = "САО РАН",
address = "Russian Federation",

}

RIS

TY - GEN

T1 - Line Profile Variability and a Possible Magnetic Field in the Spectra of Supergiant ζ Ori Aa

AU - Kholtygin, A.F.

AU - Chountonov, G.A.

AU - Dushin, V.V.

PY - 2011

Y1 - 2011

N2 - Results of spectropolarimetric observations of the supergiant ζ Ori are reported. The fast line profile variability (LPV) with a period of about 3 hours is found and a connection of LPV with a non-radial pulsation of the star is supposed. We did not find any evidence for a moderate stellar magnetic field as reported by Bouret et. al., 2008}.

AB - Results of spectropolarimetric observations of the supergiant ζ Ori are reported. The fast line profile variability (LPV) with a period of about 3 hours is found and a connection of LPV with a non-radial pulsation of the star is supposed. We did not find any evidence for a moderate stellar magnetic field as reported by Bouret et. al., 2008}.

KW - magnetic fields - stars

M3 - Conference contribution

SP - 355

EP - 360

BT - Magnetic Stars. Proceedings of the International Conference, held in the Special Astrophysical Observatory of the Russian AS, August 27- September 1, 2010, Eds: I. I. Romanyuk and D. O. Kudryavtsev

PB - САО РАН

ER -

ID: 4545531