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New Insights from Magnetic Studies of Massive OB Stars. / Kholtygin, A.; Hubrig, S.; Fabrika, S. N.; Valyavin, G.; Medvedev, A.; Chountonov, G. A.; Tsiopa, O. A.
Physics of Magnetic Stars: Proceedings of a Conference Held at Special Astrophysical Observatory, Nizhny Arkhyz, Russia, 1-5 October 2018. ред. / I.I. Romanyuk; I. A. Yakunin; D.O. Kudryavtsev. San Francisco : Astronomical Society of the Pacific, 2019. стр. 40-51 (Astronomical Society of the Pacific conference series; Том 518).
Результаты исследований: Публикации в книгах, отчётах, сборниках, трудах конференций › статья в сборнике материалов конференции › научная
Harvard
Kholtygin, A, Hubrig, S, Fabrika, SN, Valyavin, G, Medvedev, A, Chountonov, GA & Tsiopa, OA 2019,
New Insights from Magnetic Studies of Massive OB Stars. в II Romanyuk, IA Yakunin & DO Kudryavtsev (ред.),
Physics of Magnetic Stars: Proceedings of a Conference Held at Special Astrophysical Observatory, Nizhny Arkhyz, Russia, 1-5 October 2018. Astronomical Society of the Pacific conference series, Том. 518, Astronomical Society of the Pacific, San Francisco, стр. 40-51, International Conference "Physics of Magnetic Stars", Nizhny Arkhyz, Российская Федерация,
1/10/19. <
http://aspbooks.org/custom/publications/paper/518-0040.html>
APA
Kholtygin, A., Hubrig, S., Fabrika, S. N., Valyavin, G., Medvedev, A., Chountonov, G. A., & Tsiopa, O. A. (2019).
New Insights from Magnetic Studies of Massive OB Stars. в I. I. Romanyuk, I. A. Yakunin, & D. O. Kudryavtsev (Ред.),
Physics of Magnetic Stars: Proceedings of a Conference Held at Special Astrophysical Observatory, Nizhny Arkhyz, Russia, 1-5 October 2018 (стр. 40-51). (Astronomical Society of the Pacific conference series; Том 518). Astronomical Society of the Pacific.
http://aspbooks.org/custom/publications/paper/518-0040.html
Vancouver
Kholtygin A, Hubrig S, Fabrika SN, Valyavin G, Medvedev A, Chountonov GA и пр.
New Insights from Magnetic Studies of Massive OB Stars. в Romanyuk II, Yakunin IA, Kudryavtsev DO, Редакторы, Physics of Magnetic Stars: Proceedings of a Conference Held at Special Astrophysical Observatory, Nizhny Arkhyz, Russia, 1-5 October 2018. San Francisco: Astronomical Society of the Pacific. 2019. стр. 40-51. (Astronomical Society of the Pacific conference series).
Author
Kholtygin, A. ; Hubrig, S. ; Fabrika, S. N. ; Valyavin, G. ; Medvedev, A. ; Chountonov, G. A. ; Tsiopa, O. A. /
New Insights from Magnetic Studies of Massive OB Stars. Physics of Magnetic Stars: Proceedings of a Conference Held at Special Astrophysical Observatory, Nizhny Arkhyz, Russia, 1-5 October 2018. Редактор / I.I. Romanyuk ; I. A. Yakunin ; D.O. Kudryavtsev. San Francisco : Astronomical Society of the Pacific, 2019. стр. 40-51 (Astronomical Society of the Pacific conference series).
BibTeX
@inproceedings{9af5e87f76e14a18a24aeba7ee971083,
title = "New Insights from Magnetic Studies of Massive OB Stars",
abstract = "Nearly 6-7% of massive OB stars possess a magnetic field. We review recent investigations of these fields. Special attention is given to the studies of magnetic properties of high-mass X-ray binaries. A model involving the interaction of magnetized stellar wind with a neutron star magnetosphere is considered to characterize the behavior of supergiant fast X-ray transients. The presence of magnetic fields in Be stars is also discussed. We argue that the observed fraction of magnetic stars is determined by physical conditions at the pre-main-sequence stages of stellar evolution. We also consider the recent finding of fast line-profile variations on a timescale of minutes and even a fraction of a minute in spectra of OBA stars. The existence of compact regions with local magnetic fields on the surface of massive OB stars and their impact on fast line-profile variations is also discussed.",
author = "A. Kholtygin and S. Hubrig and Fabrika, {S. N.} and G. Valyavin and A. Medvedev and Chountonov, {G. A.} and Tsiopa, {O. A.}",
year = "2019",
month = jul,
day = "1",
language = "English",
isbn = "9781583819234",
series = "Astronomical Society of the Pacific conference series",
publisher = "Astronomical Society of the Pacific",
pages = "40--51",
editor = "I.I. Romanyuk and Yakunin, {I. A.} and D.O. Kudryavtsev",
booktitle = "Physics of Magnetic Stars",
address = "United States",
note = "International Conference {"}Physics of Magnetic Stars{"} ; Conference date: 01-10-2019 Through 05-10-2019",
}
RIS
TY - GEN
T1 - New Insights from Magnetic Studies of Massive OB Stars
AU - Kholtygin, A.
AU - Hubrig, S.
AU - Fabrika, S. N.
AU - Valyavin, G.
AU - Medvedev, A.
AU - Chountonov, G. A.
AU - Tsiopa, O. A.
PY - 2019/7/1
Y1 - 2019/7/1
N2 - Nearly 6-7% of massive OB stars possess a magnetic field. We review recent investigations of these fields. Special attention is given to the studies of magnetic properties of high-mass X-ray binaries. A model involving the interaction of magnetized stellar wind with a neutron star magnetosphere is considered to characterize the behavior of supergiant fast X-ray transients. The presence of magnetic fields in Be stars is also discussed. We argue that the observed fraction of magnetic stars is determined by physical conditions at the pre-main-sequence stages of stellar evolution. We also consider the recent finding of fast line-profile variations on a timescale of minutes and even a fraction of a minute in spectra of OBA stars. The existence of compact regions with local magnetic fields on the surface of massive OB stars and their impact on fast line-profile variations is also discussed.
AB - Nearly 6-7% of massive OB stars possess a magnetic field. We review recent investigations of these fields. Special attention is given to the studies of magnetic properties of high-mass X-ray binaries. A model involving the interaction of magnetized stellar wind with a neutron star magnetosphere is considered to characterize the behavior of supergiant fast X-ray transients. The presence of magnetic fields in Be stars is also discussed. We argue that the observed fraction of magnetic stars is determined by physical conditions at the pre-main-sequence stages of stellar evolution. We also consider the recent finding of fast line-profile variations on a timescale of minutes and even a fraction of a minute in spectra of OBA stars. The existence of compact regions with local magnetic fields on the surface of massive OB stars and their impact on fast line-profile variations is also discussed.
M3 - Conference contribution
SN - 9781583819234
T3 - Astronomical Society of the Pacific conference series
SP - 40
EP - 51
BT - Physics of Magnetic Stars
A2 - Romanyuk, I.I.
A2 - Yakunin, I. A.
A2 - Kudryavtsev, D.O.
PB - Astronomical Society of the Pacific
CY - San Francisco
T2 - International Conference "Physics of Magnetic Stars"
Y2 - 1 October 2019 through 5 October 2019
ER -
