Spatial Distribution of Early Spectral Type Magnetic Stars › Научные исследования в СПбГУ

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Spatial Distribution of Early Spectral Type Magnetic Stars. / Boronina, S. V.; Kholtygin, A. F.

STARS: FROM COLLAPSE TO COLLAPSE. ред. / YY Balega; DO Kudryavtsev; Romanyuk; IA Yakunin. Astronomical Society of the Pacific, 2017. стр. 270-271 (Astronomical Society of the Pacific Conference Series; Том 510).

Результаты исследований: Публикации в книгах, отчётах, сборниках, трудах конференций › статья в сборнике материалов конференции › Рецензирование

Harvard

Boronina, SV & Kholtygin, AF 2017, Spatial Distribution of Early Spectral Type Magnetic Stars. в YY Balega, DO Kudryavtsev, Romanyuk & IA Yakunin (ред.), STARS: FROM COLLAPSE TO COLLAPSE. Astronomical Society of the Pacific Conference Series, Том. 510, Astronomical Society of the Pacific, стр. 270-271, Conference on Stars: From Collapse to Collapse, Nizhny Arkhyz, 2/10/16.

APA

Boronina, S. V., & Kholtygin, A. F. (2017). Spatial Distribution of Early Spectral Type Magnetic Stars. в YY. Balega, DO. Kudryavtsev, Romanyuk, & IA. Yakunin (Ред.), STARS: FROM COLLAPSE TO COLLAPSE (стр. 270-271). (Astronomical Society of the Pacific Conference Series; Том 510). Astronomical Society of the Pacific.

Vancouver

Boronina SV, Kholtygin AF. Spatial Distribution of Early Spectral Type Magnetic Stars. в Balega YY, Kudryavtsev DO, Romanyuk, Yakunin IA, Редакторы, STARS: FROM COLLAPSE TO COLLAPSE. Astronomical Society of the Pacific. 2017. стр. 270-271. (Astronomical Society of the Pacific Conference Series).

Author

Boronina, S. V. ; Kholtygin, A. F. / Spatial Distribution of Early Spectral Type Magnetic Stars. STARS: FROM COLLAPSE TO COLLAPSE. Редактор / YY Balega ; DO Kudryavtsev ; Romanyuk ; IA Yakunin. Astronomical Society of the Pacific, 2017. стр. 270-271 (Astronomical Society of the Pacific Conference Series).

BibTeX

@inproceedings{e9020d08c1ff45f49a4f90878e628354,

title = "Spatial Distribution of Early Spectral Type Magnetic Stars",

abstract = "We have taken O, B, A and F magnetic stars from the catalog by Bychkov et. al (2009) and divided them into three groups: stars with the rms magnetic field strength ⟨B⟩e> 100G was accepted as {"}suspected to be magnetic{"}. Some of the {"}suspected to be magnetic{"} stars satisfying both conditions ⟨B⟩e>2σ and χ2>1 were considered to be magnetic. The galactic coordinates and other parameters of all O, B, A, and F type stars were taken from SIMBAD. The spatial and surface densities of all considered types of stars were calculated. ",

author = "Boronina, {S. V.} and Kholtygin, {A. F.}",

year = "2017",

language = "Английский",

isbn = "978-1-58381-904-3",

series = "Astronomical Society of the Pacific Conference Series",

publisher = "Astronomical Society of the Pacific",

pages = "270--271",

editor = "YY Balega and DO Kudryavtsev and Romanyuk and IA Yakunin",

booktitle = "STARS: FROM COLLAPSE TO COLLAPSE",

address = "Соединенные Штаты Америки",

note = "null ; Conference date: 02-10-2016 Through 06-10-2016",

}

RIS

TY - GEN

T1 - Spatial Distribution of Early Spectral Type Magnetic Stars

AU - Boronina, S. V.

AU - Kholtygin, A. F.

PY - 2017

Y1 - 2017

N2 - We have taken O, B, A and F magnetic stars from the catalog by Bychkov et. al (2009) and divided them into three groups: stars with the rms magnetic field strength ⟨B⟩e> 100G was accepted as "suspected to be magnetic". Some of the "suspected to be magnetic" stars satisfying both conditions ⟨B⟩e>2σ and χ2>1 were considered to be magnetic. The galactic coordinates and other parameters of all O, B, A, and F type stars were taken from SIMBAD. The spatial and surface densities of all considered types of stars were calculated.

AB - We have taken O, B, A and F magnetic stars from the catalog by Bychkov et. al (2009) and divided them into three groups: stars with the rms magnetic field strength ⟨B⟩e> 100G was accepted as "suspected to be magnetic". Some of the "suspected to be magnetic" stars satisfying both conditions ⟨B⟩e>2σ and χ2>1 were considered to be magnetic. The galactic coordinates and other parameters of all O, B, A, and F type stars were taken from SIMBAD. The spatial and surface densities of all considered types of stars were calculated.

M3 - статья в сборнике материалов конференции

SN - 978-1-58381-904-3

T3 - Astronomical Society of the Pacific Conference Series

SP - 270

EP - 271

BT - STARS: FROM COLLAPSE TO COLLAPSE

A2 - Balega, YY

A2 - Kudryavtsev, DO

A2 - Romanyuk, null

A2 - Yakunin, IA

PB - Astronomical Society of the Pacific

Y2 - 2 October 2016 through 6 October 2016

ER -

ID: 9366566