The Role of Damped Alfven Waves in Magnetospheric Accretion Models of Young Stars
Author:
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://stacks.iop.org/0004-637X/574/i=2/a=847/pdf
Reference49 articles.
1. Profiles of Strong Permitted Lines in Classical T Tauri Stars
2. Electron density power spectrum in the local interstellar medium
3. [ITAL]Hubble Space Telescope[/ITAL] STIS Spectroscopy of the Optical Outflow from DG Tauri: Structure and Kinematics on Subarcsecond Scales
4. Instability, turbulence, and enhanced transport in accretion disks
Cited by 5 articles. 订阅此论文施引文献 订阅此论文施引文献，注册后可以免费订阅5篇论文的施引文献，订阅后可以查看论文全部施引文献
1. Turbulence‐driven Polar Winds from T Tauri Stars Energized by Magnetospheric Accretion;The Astrophysical Journal;2008-12-10
2. Global Alfven Wave Heating of the Magnetosphere of Young Stars;The Astrophysical Journal;2004-01
3. Alfven waves in the context of solar-like star formation: Accretion columns and disks;Space Science Reviews;2003
4. Alfven Waves in Disks, Outflows and Jets;Open Issues in Local Star Formation;2003
5. Alfvén Waves in the Context of Solar-Like Star Formation: Accretion Columns and Disks;Advances in Space Environment Research - Volume I;2003
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