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Large-scale magnetic field of the accretion disks of T Tauri stars. / Dudorov, Alexander; Khaibrakhmanov, Sergey; Parfenov, Sergey и др.
в: Proceedings of the International Astronomical Union, Том 14, № S345, 2018, стр. 297-298.

Результаты исследований: Вклад в журналМатериалы конференцииРецензирование

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Dudorov A, Khaibrakhmanov S, Parfenov S, Sobolev A. Large-scale magnetic field of the accretion disks of T Tauri stars. Proceedings of the International Astronomical Union. 2018;14(S345):297-298. doi: 10.1017/S1743921319001443

Author

Dudorov, Alexander ; Khaibrakhmanov, Sergey ; Parfenov, Sergey и др. / Large-scale magnetic field of the accretion disks of T Tauri stars. в: Proceedings of the International Astronomical Union. 2018 ; Том 14, № S345. стр. 297-298.

BibTeX

@article{d11d98c59df948a79b2b5697ca37a773,
title = "Large-scale magnetic field of the accretion disks of T Tauri stars",
abstract = "The large-scale magnetic field in the accretion disks of young stars is investigated. Main features of our magnetohydrodynamical (MHD) model of the accretion disks and typical simulation results are presented. We discuss the role of MHD effects, ionization structure, magnetic field geometry and strength of the accretion disks. {\textcopyright} International Astronomical Union 2020.",
author = "Alexander Dudorov and Sergey Khaibrakhmanov and Sergey Parfenov and Andrey Sobolev",
year = "2018",
doi = "10.1017/S1743921319001443",
language = "English",
volume = "14",
pages = "297--298",
journal = "Proceedings of the International Astronomical Union",
issn = "1743-9213",
publisher = "Cambridge University Press",
number = "S345",

}

RIS

TY - JOUR

T1 - Large-scale magnetic field of the accretion disks of T Tauri stars

AU - Dudorov, Alexander

AU - Khaibrakhmanov, Sergey

AU - Parfenov, Sergey

AU - Sobolev, Andrey

PY - 2018

Y1 - 2018

N2 - The large-scale magnetic field in the accretion disks of young stars is investigated. Main features of our magnetohydrodynamical (MHD) model of the accretion disks and typical simulation results are presented. We discuss the role of MHD effects, ionization structure, magnetic field geometry and strength of the accretion disks. © International Astronomical Union 2020.

AB - The large-scale magnetic field in the accretion disks of young stars is investigated. Main features of our magnetohydrodynamical (MHD) model of the accretion disks and typical simulation results are presented. We discuss the role of MHD effects, ionization structure, magnetic field geometry and strength of the accretion disks. © International Astronomical Union 2020.

UR - http://www.scopus.com/inward/record.url?partnerID=8YFLogxK&scp=85077981007

U2 - 10.1017/S1743921319001443

DO - 10.1017/S1743921319001443

M3 - Conference article

VL - 14

SP - 297

EP - 298

JO - Proceedings of the International Astronomical Union

JF - Proceedings of the International Astronomical Union

SN - 1743-9213

IS - S345

ER -

ID: 57309504