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On the Magnetic Field Structure of Chemically Peculiar Star 53 Cam. / Romanyuk, I. I.; Moiseeva, A. V.; Kudryavtsev, D. O.; Yakunin, I. A.; Aitov, V. N.; Baklanova, D. N.

в: Astrophysical Bulletin, Том 77, № 2, 01.06.2022, стр. 156-166.

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

Harvard

Romanyuk, II, Moiseeva, AV, Kudryavtsev, DO, Yakunin, IA, Aitov, VN & Baklanova, DN 2022, 'On the Magnetic Field Structure of Chemically Peculiar Star 53 Cam', Astrophysical Bulletin, Том. 77, № 2, стр. 156-166. https://doi.org/10.1134/S1990341322020080

APA

Romanyuk, I. I., Moiseeva, A. V., Kudryavtsev, D. O., Yakunin, I. A., Aitov, V. N., & Baklanova, D. N. (2022). On the Magnetic Field Structure of Chemically Peculiar Star 53 Cam. Astrophysical Bulletin, 77(2), 156-166. https://doi.org/10.1134/S1990341322020080

Vancouver

Romanyuk II, Moiseeva AV, Kudryavtsev DO, Yakunin IA, Aitov VN, Baklanova DN. On the Magnetic Field Structure of Chemically Peculiar Star 53 Cam. Astrophysical Bulletin. 2022 Июнь 1;77(2):156-166. https://doi.org/10.1134/S1990341322020080

Author

Romanyuk, I. I. ; Moiseeva, A. V. ; Kudryavtsev, D. O. ; Yakunin, I. A. ; Aitov, V. N. ; Baklanova, D. N. / On the Magnetic Field Structure of Chemically Peculiar Star 53 Cam. в: Astrophysical Bulletin. 2022 ; Том 77, № 2. стр. 156-166.

BibTeX

@article{c289f2ef1449445fa695d727361238a9,
title = "On the Magnetic Field Structure of Chemically Peculiar Star 53 Cam",
abstract = "Abstract—Based on our previous and recent magnetic field observations of a chemically peculiar star 53 Cam with the 6-m telescope and literary sources, we can make a conclusion that its magnetic field structure differs from a simple dipole. At the same time the results of measurements from hydrogen lines are described by a simple dipole model. However, data obtained from metallic lines (including magnetic mapping methods) point to a more complex field structure. We performed new observations of the magnetic field in the Balmer series hydrogen lines in the near UV-range. These peculiarities may show that the field strength increases with depth in the atmosphere of 53 Cam.",
keywords = "stars: chemically peculiar, stars: individual: 53 Cam, stars: magnetic field",
author = "Romanyuk, {I. I.} and Moiseeva, {A. V.} and Kudryavtsev, {D. O.} and Yakunin, {I. A.} and Aitov, {V. N.} and Baklanova, {D. N.}",
year = "2022",
month = jun,
day = "1",
doi = "10.1134/S1990341322020080",
language = "English",
volume = "77",
pages = "156--166",
journal = "Astrophysical Bulletin",
issn = "1990-3413",
publisher = "МАИК {"}Наука/Интерпериодика{"}",
number = "2",

}

RIS

TY - JOUR

T1 - On the Magnetic Field Structure of Chemically Peculiar Star 53 Cam

AU - Romanyuk, I. I.

AU - Moiseeva, A. V.

AU - Kudryavtsev, D. O.

AU - Yakunin, I. A.

AU - Aitov, V. N.

AU - Baklanova, D. N.

PY - 2022/6/1

Y1 - 2022/6/1

N2 - Abstract—Based on our previous and recent magnetic field observations of a chemically peculiar star 53 Cam with the 6-m telescope and literary sources, we can make a conclusion that its magnetic field structure differs from a simple dipole. At the same time the results of measurements from hydrogen lines are described by a simple dipole model. However, data obtained from metallic lines (including magnetic mapping methods) point to a more complex field structure. We performed new observations of the magnetic field in the Balmer series hydrogen lines in the near UV-range. These peculiarities may show that the field strength increases with depth in the atmosphere of 53 Cam.

AB - Abstract—Based on our previous and recent magnetic field observations of a chemically peculiar star 53 Cam with the 6-m telescope and literary sources, we can make a conclusion that its magnetic field structure differs from a simple dipole. At the same time the results of measurements from hydrogen lines are described by a simple dipole model. However, data obtained from metallic lines (including magnetic mapping methods) point to a more complex field structure. We performed new observations of the magnetic field in the Balmer series hydrogen lines in the near UV-range. These peculiarities may show that the field strength increases with depth in the atmosphere of 53 Cam.

KW - stars: chemically peculiar

KW - stars: individual: 53 Cam

KW - stars: magnetic field

UR - http://www.scopus.com/inward/record.url?scp=85133443230&partnerID=8YFLogxK

U2 - 10.1134/S1990341322020080

DO - 10.1134/S1990341322020080

M3 - Article

AN - SCOPUS:85133443230

VL - 77

SP - 156

EP - 166

JO - Astrophysical Bulletin

JF - Astrophysical Bulletin

SN - 1990-3413

IS - 2

ER -

ID: 126868777