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Large-scale magnetic field of the accretion disks of T Tauri stars
Published online by Cambridge University Press: 13 January 2020
Abstract
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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.
- Type
- Contributed Papers
- Information
- Proceedings of the International Astronomical Union , Volume 14 , Symposium S345: Origins: From the Protosun to the First Steps of Life , August 2018 , pp. 297 - 298
- Copyright
- © International Astronomical Union 2020
References
Khaibrakhmanov, S. A., Dudorov, A. E., Parfenov, S. Yu., & Sobolev, A. M. 2017, MNRAS, 464, 586
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