JET FORMATION FROM MASSIVE YOUNG STARS: MAGNETOHYDRODYNAMICS VERSUS RADIATION PRESSURE
Author:
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://stacks.iop.org/0004-637X/742/i=1/a=56/pdf
Reference66 articles.
1. The theory of radiatively driven stellar winds. II - The line acceleration
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3. Observations and Modeling of the Inner Disk Region of T Tauri Stars
4. Locating the Launching Region of T Tauri Winds: The Case of DG Tauri
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