Damping of Alfvén waves as a heating source in protostellar accretion discs
Author:
Publisher
Oxford University Press (OUP)
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://academic.oup.com/mnras/article-pdf/431/4/3150/3937530/stt397.pdf
Reference52 articles.
1. The Birth Environment of the Solar System
2. Infrared spectra of rotating protostars
3. High‐Resolution Submillimeter Constraints on Circumstellar Disk Structure
4. A powerful local shear instability in weakly magnetized disks. I - Linear analysis. II - Nonlinear evolution
5. Using FU Orionis outbursts to constrain self-regulated protostellar disk models
Cited by 2 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. The dead zone size limits in a proto-stellar accretion disc model heated by the damping of Alfvén waves;Astrophysics and Space Science;2015-04-18
2. Alfvén waves in space and astrophysical dusty plasmas;Nonlinear Processes in Geophysics;2014-03-13
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