Standard

Magnetic stars with wide depressions in the continuum. 2. The silicon star with a complex field structure HD 27404. / Semenko, E. A.; Romanyuk, I. I.; Moiseeva, A. V.; Kudryavtsev, D. O.; Yakunin, I. A.

в: Astrophysical Bulletin, Том 72, № 4, 01.10.2017, стр. 384-390.

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

Harvard

Semenko, EA, Romanyuk, II, Moiseeva, AV, Kudryavtsev, DO & Yakunin, IA 2017, 'Magnetic stars with wide depressions in the continuum. 2. The silicon star with a complex field structure HD 27404', Astrophysical Bulletin, Том. 72, № 4, стр. 384-390. https://doi.org/10.1134/S1990341317040034

APA

Semenko, E. A., Romanyuk, I. I., Moiseeva, A. V., Kudryavtsev, D. O., & Yakunin, I. A. (2017). Magnetic stars with wide depressions in the continuum. 2. The silicon star with a complex field structure HD 27404. Astrophysical Bulletin, 72(4), 384-390. https://doi.org/10.1134/S1990341317040034

Vancouver

Semenko EA, Romanyuk II, Moiseeva AV, Kudryavtsev DO, Yakunin IA. Magnetic stars with wide depressions in the continuum. 2. The silicon star with a complex field structure HD 27404. Astrophysical Bulletin. 2017 Окт. 1;72(4):384-390. https://doi.org/10.1134/S1990341317040034

Author

Semenko, E. A. ; Romanyuk, I. I. ; Moiseeva, A. V. ; Kudryavtsev, D. O. ; Yakunin, I. A. / Magnetic stars with wide depressions in the continuum. 2. The silicon star with a complex field structure HD 27404. в: Astrophysical Bulletin. 2017 ; Том 72, № 4. стр. 384-390.

BibTeX

@article{be0ea6ee4b0c47e09eb636306e84db65,
title = "Magnetic stars with wide depressions in the continuum. 2. The silicon star with a complex field structure HD 27404",
abstract = "Observations of the chemically peculiar star HD 27404 with the 6-m SAO RAS telescope showed a strong magnetic field with the longitudinal field component varying in a complicated way in the range of −2.5 to 1 kG. Fundamental parameters of the star (Teff = 11 300 K, log g = 3.9) were estimated analyzing photometric indices in the Geneva and in the Stromgren–Crawford photometric systems. We detected weak radial velocity variations which can be due to the presence of a close star companion or chemical spots in the photosphere. Rapid estimation of the key chemical element abundance allows us to refer HD 27404 to a SiCr or Si+ chemically peculiar A0–B9 star.",
keywords = "chemically peculiar—stars, HD 27404, individual, magnetic field—stars, stars",
author = "Semenko, {E. A.} and Romanyuk, {I. I.} and Moiseeva, {A. V.} and Kudryavtsev, {D. O.} and Yakunin, {I. A.}",
year = "2017",
month = oct,
day = "1",
doi = "10.1134/S1990341317040034",
language = "English",
volume = "72",
pages = "384--390",
journal = "Astrophysical Bulletin",
issn = "1990-3413",
publisher = "МАИК {"}Наука/Интерпериодика{"}",
number = "4",

}

RIS

TY - JOUR

T1 - Magnetic stars with wide depressions in the continuum. 2. The silicon star with a complex field structure HD 27404

AU - Semenko, E. A.

AU - Romanyuk, I. I.

AU - Moiseeva, A. V.

AU - Kudryavtsev, D. O.

AU - Yakunin, I. A.

PY - 2017/10/1

Y1 - 2017/10/1

N2 - Observations of the chemically peculiar star HD 27404 with the 6-m SAO RAS telescope showed a strong magnetic field with the longitudinal field component varying in a complicated way in the range of −2.5 to 1 kG. Fundamental parameters of the star (Teff = 11 300 K, log g = 3.9) were estimated analyzing photometric indices in the Geneva and in the Stromgren–Crawford photometric systems. We detected weak radial velocity variations which can be due to the presence of a close star companion or chemical spots in the photosphere. Rapid estimation of the key chemical element abundance allows us to refer HD 27404 to a SiCr or Si+ chemically peculiar A0–B9 star.

AB - Observations of the chemically peculiar star HD 27404 with the 6-m SAO RAS telescope showed a strong magnetic field with the longitudinal field component varying in a complicated way in the range of −2.5 to 1 kG. Fundamental parameters of the star (Teff = 11 300 K, log g = 3.9) were estimated analyzing photometric indices in the Geneva and in the Stromgren–Crawford photometric systems. We detected weak radial velocity variations which can be due to the presence of a close star companion or chemical spots in the photosphere. Rapid estimation of the key chemical element abundance allows us to refer HD 27404 to a SiCr or Si+ chemically peculiar A0–B9 star.

KW - chemically peculiar—stars

KW - HD 27404

KW - individual

KW - magnetic field—stars

KW - stars

UR - http://www.scopus.com/inward/record.url?scp=85035212065&partnerID=8YFLogxK

U2 - 10.1134/S1990341317040034

DO - 10.1134/S1990341317040034

M3 - Article

AN - SCOPUS:85035212065

VL - 72

SP - 384

EP - 390

JO - Astrophysical Bulletin

JF - Astrophysical Bulletin

SN - 1990-3413

IS - 4

ER -

ID: 127695033