Результаты исследований: Научные публикации в периодических изданиях › статья › Рецензирование
Results of Magnetic-Field Measurements with the 6-m Telescope. V. Observations in 2011. / Romanyuk, I. I.; Semenko, E. A.; Moiseeva, A. V.; Kudryavtsev, D. O.; Yakunin, I. A.
в: Astrophysical Bulletin, Том 73, № 2, 01.04.2018, стр. 178-200.Результаты исследований: Научные публикации в периодических изданиях › статья › Рецензирование
}
TY - JOUR
T1 - Results of Magnetic-Field Measurements with the 6-m Telescope. V. Observations in 2011
AU - Romanyuk, I. I.
AU - Semenko, E. A.
AU - Moiseeva, A. V.
AU - Kudryavtsev, D. O.
AU - Yakunin, I. A.
PY - 2018/4/1
Y1 - 2018/4/1
N2 - The paper presents results of measurements of magnetic-field longitudinal components Be, radial velocities Vr, and projections of the rotation velocity in the line of sight ve sin i for 74 objects, mainly main-sequence chemically peculiar stars and standard stars. Observations were carried out in 2011 at the 6-m BTA telescope using the Main Stellar Spectrograph (MSS) with a Zeeman analyzer. Seven new magnetic stars were discovered: HD38129, HD47152, HD50341, HD63347, HD188501, HD191287, and HD260858. Three more stars were suspected to have magnetic fields. Observations of magnetic standard stars and non-magnetic stars confirm the absence of any systematic errors capable of introducing distortions into the Be longitudinal-field measurement results. The paper gives comments on the research results for each of the 74 stars.
AB - The paper presents results of measurements of magnetic-field longitudinal components Be, radial velocities Vr, and projections of the rotation velocity in the line of sight ve sin i for 74 objects, mainly main-sequence chemically peculiar stars and standard stars. Observations were carried out in 2011 at the 6-m BTA telescope using the Main Stellar Spectrograph (MSS) with a Zeeman analyzer. Seven new magnetic stars were discovered: HD38129, HD47152, HD50341, HD63347, HD188501, HD191287, and HD260858. Three more stars were suspected to have magnetic fields. Observations of magnetic standard stars and non-magnetic stars confirm the absence of any systematic errors capable of introducing distortions into the Be longitudinal-field measurement results. The paper gives comments on the research results for each of the 74 stars.
KW - stars: chemically peculiar
KW - stars: magnetic field
UR - http://www.scopus.com/inward/record.url?scp=85047853262&partnerID=8YFLogxK
U2 - 10.1134/S1990341318020050
DO - 10.1134/S1990341318020050
M3 - Article
AN - SCOPUS:85047853262
VL - 73
SP - 178
EP - 200
JO - Astrophysical Bulletin
JF - Astrophysical Bulletin
SN - 1990-3413
IS - 2
ER -
ID: 126869233