Magnetically Fed Hot Star Keplerian Disks with Slow Outflow-Reference-Cited by-同舟云学术

Magnetically Fed Hot Star Keplerian Disks with Slow Outflow

Published:2008-12 Issue:2 Volume:688 Page:1320-1325
ISSN:0004-637X
Container-title:The Astrophysical Journal
language:en
Short-container-title:Astrophysical Journal

Author:

Brown J. C.,Cassinelli J. P.,Maheswaran M.

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference43 articles.

1. A powerful local shear instability in weakly magnetized disks. I - Linear analysis. II - Nonlinear evolution

2. Nonlinear Stability, Hydrodynamical Turbulence, and Transport in Disks

3. Equatorial disk formation around rotating stars due to Ram pressure confinement by the stellar wind

4. Brown, J. C. & Cassinelli, J. P. 2005, in ASP Conf. Ser. 337, The Nature and Evolution of Disks around Hot Stars, ed. R. Ignace & K. G. Gayley (San Francisco: ASP), 88

5. The effect of rotational gravity darkening on magnetically torqued Be star discs

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