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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. ed. / I.I. Romanyuk; I. A. Yakunin; D.O. Kudryavtsev. San Francisco : Astronomical Society of the Pacific, 2019. p. 40-51 (Astronomical Society of the Pacific conference series; Vol. 518).
Research output: Chapter in Book/Report/Conference proceeding › Conference contribution
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. in II Romanyuk, IA Yakunin & DO Kudryavtsev (eds),
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, vol. 518, Astronomical Society of the Pacific, San Francisco, pp. 40-51, International Conference "Physics of Magnetic Stars", Nizhny Arkhyz, Russian Federation,
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. In I. I. Romanyuk, I. A. Yakunin, & D. O. Kudryavtsev (Eds.),
Physics of Magnetic Stars: Proceedings of a Conference Held at Special Astrophysical Observatory, Nizhny Arkhyz, Russia, 1-5 October 2018 (pp. 40-51). (Astronomical Society of the Pacific conference series; Vol. 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 et al.
New Insights from Magnetic Studies of Massive OB Stars. In Romanyuk II, Yakunin IA, Kudryavtsev DO, editors, 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. p. 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. editor / I.I. Romanyuk ; I. A. Yakunin ; D.O. Kudryavtsev. San Francisco : Astronomical Society of the Pacific, 2019. pp. 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 -
