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Rising magnetic flux tubes as a source of IR-variability of the accretion disks of young stars. / Khaibrakhmanov, Sergey A.; Dudorov, Alexander E.; Sobolev, Andrey M.

в: Proceedings of the International Astronomical Union, 01.01.2019, стр. 295-296.

Результаты исследований: Научные публикации в периодических изданиях › статья › Рецензирование

Harvard

Khaibrakhmanov, SA, Dudorov, AE & Sobolev, AM 2019, 'Rising magnetic flux tubes as a source of IR-variability of the accretion disks of young stars', Proceedings of the International Astronomical Union, стр. 295-296. https://doi.org/10.1017/S1743921319001431

APA

Khaibrakhmanov, S. A., Dudorov, A. E., & Sobolev, A. M. (2019). Rising magnetic flux tubes as a source of IR-variability of the accretion disks of young stars. Proceedings of the International Astronomical Union, 295-296. https://doi.org/10.1017/S1743921319001431

Vancouver

Khaibrakhmanov SA, Dudorov AE, Sobolev AM. Rising magnetic flux tubes as a source of IR-variability of the accretion disks of young stars. Proceedings of the International Astronomical Union. 2019 Янв. 1;295-296. https://doi.org/10.1017/S1743921319001431

Author

Khaibrakhmanov, Sergey A. ; Dudorov, Alexander E. ; Sobolev, Andrey M. / Rising magnetic flux tubes as a source of IR-variability of the accretion disks of young stars. в: Proceedings of the International Astronomical Union. 2019 ; стр. 295-296.

BibTeX

@article{e47571e9de20400eb1d3bd51c4a42438,
title = "Rising magnetic flux tubes as a source of IR-variability of the accretion disks of young stars",
abstract = "We investigate dynamics of slender magnetic flux tubes (MFT) in the accretion disks of young stars. Simulations show that MFT rise from the disk and can accelerate to 20-30 km/s causing periodic outflows. Magnetic field of the disk counteracts the buoyancy, and the MFT oscillate near the disk's surface with periods of 10-100 days. We demonstrate that rising and oscillating MFT can cause the IR-variability of the accretion disks of young stars.",
keywords = "Accretion, accretion disks, infrared: ISM, instabilities, ISM: jets and outflows, ISM: magnetic fields, MHD",
author = "Khaibrakhmanov, {Sergey A.} and Dudorov, {Alexander E.} and Sobolev, {Andrey M.}",
year = "2019",
month = jan,
day = "1",
doi = "10.1017/S1743921319001431",
language = "English",
pages = "295--296",
journal = "Proceedings of the International Astronomical Union",
issn = "1743-9213",
publisher = "Cambridge University Press",

}

RIS

TY - JOUR

T1 - Rising magnetic flux tubes as a source of IR-variability of the accretion disks of young stars

AU - Khaibrakhmanov, Sergey A.

AU - Dudorov, Alexander E.

AU - Sobolev, Andrey M.

PY - 2019/1/1

Y1 - 2019/1/1

N2 - We investigate dynamics of slender magnetic flux tubes (MFT) in the accretion disks of young stars. Simulations show that MFT rise from the disk and can accelerate to 20-30 km/s causing periodic outflows. Magnetic field of the disk counteracts the buoyancy, and the MFT oscillate near the disk's surface with periods of 10-100 days. We demonstrate that rising and oscillating MFT can cause the IR-variability of the accretion disks of young stars.

AB - We investigate dynamics of slender magnetic flux tubes (MFT) in the accretion disks of young stars. Simulations show that MFT rise from the disk and can accelerate to 20-30 km/s causing periodic outflows. Magnetic field of the disk counteracts the buoyancy, and the MFT oscillate near the disk's surface with periods of 10-100 days. We demonstrate that rising and oscillating MFT can cause the IR-variability of the accretion disks of young stars.

KW - Accretion

KW - accretion disks

KW - infrared: ISM

KW - instabilities

KW - ISM: jets and outflows

KW - ISM: magnetic fields

KW - MHD

UR - http://www.scopus.com/inward/record.url?scp=85078022359&partnerID=8YFLogxK

U2 - 10.1017/S1743921319001431

DO - 10.1017/S1743921319001431

M3 - Article

AN - SCOPUS:85078022359

SP - 295

EP - 296

JO - Proceedings of the International Astronomical Union

JF - Proceedings of the International Astronomical Union

SN - 1743-9213

ER -

ID: 103443480