Research output: Contribution to journal › Article › peer-review
Results of magnetic field measurements performed with the 6-m telescope. IV. Observations in 2010. / Romanyuk, I. I.; Semenko, E. A.; Kudryavtsev, D. O.; Moiseeva, A. V.; Yakunin, I. A.
In: Astrophysical Bulletin, Vol. 72, No. 4, 01.10.2017, p. 391-410.Research output: Contribution to journal › Article › peer-review
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TY - JOUR
T1 - Results of magnetic field measurements performed with the 6-m telescope. IV. Observations in 2010
AU - Romanyuk, I. I.
AU - Semenko, E. A.
AU - Kudryavtsev, D. O.
AU - Moiseeva, A. V.
AU - Yakunin, I. A.
PY - 2017/10/1
Y1 - 2017/10/1
N2 - We present the results of measurements of magnetic fields, radial velocities and rotation velocities for 92 objects, mainly main-sequence chemically peculiar stars. Observations were performed at the 6-m BTA telescope using Main Stellar Spectrograph with a Zeeman analyzer. In 2010, twelve new magnetic stars were discovered: HD 17330, HD 29762, HD 49884, HD 54824, HD 89069, HD 96003, HD 113894, HD 118054, HD 135679, HD 138633, HD 138777, BD +53.1183. The presence of a field is suspected in HD 16705, HD 35379 and HD 35881. Observations of standard stars without a magnetic field confirm the absence of systematic errors which can introduce distortions into the measurements of longitudinal field. The paper gives comments on the results of investigation of each star.
AB - We present the results of measurements of magnetic fields, radial velocities and rotation velocities for 92 objects, mainly main-sequence chemically peculiar stars. Observations were performed at the 6-m BTA telescope using Main Stellar Spectrograph with a Zeeman analyzer. In 2010, twelve new magnetic stars were discovered: HD 17330, HD 29762, HD 49884, HD 54824, HD 89069, HD 96003, HD 113894, HD 118054, HD 135679, HD 138633, HD 138777, BD +53.1183. The presence of a field is suspected in HD 16705, HD 35379 and HD 35881. Observations of standard stars without a magnetic field confirm the absence of systematic errors which can introduce distortions into the measurements of longitudinal field. The paper gives comments on the results of investigation of each star.
KW - chemically peculiar
KW - magnetic field—stars
KW - stars
UR - http://www.scopus.com/inward/record.url?scp=85035225590&partnerID=8YFLogxK
U2 - 10.1134/S1990341317040046
DO - 10.1134/S1990341317040046
M3 - Article
AN - SCOPUS:85035225590
VL - 72
SP - 391
EP - 410
JO - Astrophysical Bulletin
JF - Astrophysical Bulletin
SN - 1990-3413
IS - 4
ER -
ID: 126869419