Standard
Possible Detection of a Magnetic Field in X Persei. / Valyavin, G.; Ikhsanov, N. R.; Beskrovnaya, N. G.; Gadelshin, D.; Galazutdinov, G. A.; Semenko, E.; Romanyuk, I. I.; Kholtygin, A. F.; Sabin, L.; Hiriart, D.; Chountonov, G.
STARS: FROM COLLAPSE TO COLLAPSE. ed. / YY Balega; DO Kudryavtsev; Romanyuk; IA Yakunin. Astronomical Society of the Pacific, 2017. p. 229-232 (Astronomical Society of the Pacific Conference Series; Vol. 510).
Research output: Chapter in Book/Report/Conference proceeding › Conference contribution › peer-review
Harvard
Valyavin, G
, Ikhsanov, NR, Beskrovnaya, NG, Gadelshin, D, Galazutdinov, GA, Semenko, E, Romanyuk, II
, Kholtygin, AF, Sabin, L, Hiriart, D & Chountonov, G 2017,
Possible Detection of a Magnetic Field in X Persei. in YY Balega, DO Kudryavtsev, Romanyuk & IA Yakunin (eds),
STARS: FROM COLLAPSE TO COLLAPSE. Astronomical Society of the Pacific Conference Series, vol. 510, Astronomical Society of the Pacific, pp. 229-232, Conference on Stars: From Collapse to Collapse, Nizhny Arkhyz,
2/10/16.
APA
Valyavin, G.
, Ikhsanov, N. R., Beskrovnaya, N. G., Gadelshin, D., Galazutdinov, G. A., Semenko, E., Romanyuk, I. I.
, Kholtygin, A. F., Sabin, L., Hiriart, D., & Chountonov, G. (2017).
Possible Detection of a Magnetic Field in X Persei. In YY. Balega, DO. Kudryavtsev, Romanyuk, & IA. Yakunin (Eds.),
STARS: FROM COLLAPSE TO COLLAPSE (pp. 229-232). (Astronomical Society of the Pacific Conference Series; Vol. 510). Astronomical Society of the Pacific.
Vancouver
Valyavin G
, Ikhsanov NR, Beskrovnaya NG, Gadelshin D, Galazutdinov GA, Semenko E et al.
Possible Detection of a Magnetic Field in X Persei. In Balega YY, Kudryavtsev DO, Romanyuk, Yakunin IA, editors, STARS: FROM COLLAPSE TO COLLAPSE. Astronomical Society of the Pacific. 2017. p. 229-232. (Astronomical Society of the Pacific Conference Series).
Author
Valyavin, G.
; Ikhsanov, N. R. ; Beskrovnaya, N. G. ; Gadelshin, D. ; Galazutdinov, G. A. ; Semenko, E. ; Romanyuk, I. I.
; Kholtygin, A. F. ; Sabin, L. ; Hiriart, D. ; Chountonov, G. /
Possible Detection of a Magnetic Field in X Persei. STARS: FROM COLLAPSE TO COLLAPSE. editor / YY Balega ; DO Kudryavtsev ; Romanyuk ; IA Yakunin. Astronomical Society of the Pacific, 2017. pp. 229-232 (Astronomical Society of the Pacific Conference Series).
BibTeX
@inproceedings{d0adf0860cdc460eb8f994646394364b,
title = "Possible Detection of a Magnetic Field in X Persei",
abstract = "We present the results of magnetometric observations of the classic high mass X-ray binary star X Persei. Analysing magnetically-induced circular polarization in the strong emission spectral features, we have detected the presence of a variable longitudinal magnetic field in this star. The field varies from -413 ±100 G to +491± 130 G with the average value -161±113 G and period P ≍ 0.7 days. We interpret this period to be due to the spin rotation of the star. A combined analysis of absorption spectral lines revealed no field.",
keywords = "RAY, SPECTRUM, PERIOD, STARS",
author = "G. Valyavin and Ikhsanov, {N. R.} and Beskrovnaya, {N. G.} and D. Gadelshin and Galazutdinov, {G. A.} and E. Semenko and Romanyuk, {I. I.} and Kholtygin, {A. F.} and L. Sabin and D. Hiriart and G. Chountonov",
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 = "229--232",
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 - Possible Detection of a Magnetic Field in X Persei
AU - Valyavin, G.
AU - Ikhsanov, N. R.
AU - Beskrovnaya, N. G.
AU - Gadelshin, D.
AU - Galazutdinov, G. A.
AU - Semenko, E.
AU - Romanyuk, I. I.
AU - Kholtygin, A. F.
AU - Sabin, L.
AU - Hiriart, D.
AU - Chountonov, G.
PY - 2017
Y1 - 2017
N2 - We present the results of magnetometric observations of the classic high mass X-ray binary star X Persei. Analysing magnetically-induced circular polarization in the strong emission spectral features, we have detected the presence of a variable longitudinal magnetic field in this star. The field varies from -413 ±100 G to +491± 130 G with the average value -161±113 G and period P ≍ 0.7 days. We interpret this period to be due to the spin rotation of the star. A combined analysis of absorption spectral lines revealed no field.
AB - We present the results of magnetometric observations of the classic high mass X-ray binary star X Persei. Analysing magnetically-induced circular polarization in the strong emission spectral features, we have detected the presence of a variable longitudinal magnetic field in this star. The field varies from -413 ±100 G to +491± 130 G with the average value -161±113 G and period P ≍ 0.7 days. We interpret this period to be due to the spin rotation of the star. A combined analysis of absorption spectral lines revealed no field.
KW - RAY
KW - SPECTRUM
KW - PERIOD
KW - STARS
M3 - статья в сборнике материалов конференции
SN - 978-1-58381-904-3
T3 - Astronomical Society of the Pacific Conference Series
SP - 229
EP - 232
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 -
